ijaz ahmed ijaz ahmed helmut burkhardt andrea latina beam-halo generation study in clic clic beam...
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Ijaz AhmedIjaz Ahmed
Helmut BurkhardtHelmut Burkhardt
Andrea LatinaAndrea Latina
Beam-Halo Generation Study in Beam-Halo Generation Study in CLICCLIC
CLIC Beam Dynamics Meeting CERN 130208CLIC Beam Dynamics Meeting CERN 130208
Collimation SystemCollimation System
(1) Reduce the background by removing particles at large (1) Reduce the background by removing particles at large betatron amplitudes betatron amplitudes (Halo)(Halo) or energy Offsets or energy Offsets
(2) The choice of the collimator apertures should guarantee (2) The choice of the collimator apertures should guarantee good cleaning efficiency of good cleaning efficiency of HaloHalo
(3) to avoid wakefields that might degrade the orbit stability(3) to avoid wakefields that might degrade the orbit stability
Final Focus SystemFinal Focus System
(1)(1) Need to provide a very strong focusingNeed to provide a very strong focusing(2)(2) Reduces the transverse sizes of the beam at the IP Reduces the transverse sizes of the beam at the IP
sufficiently to provide the required luminositysufficiently to provide the required luminosity(3)(3) The correction of chromatic and geometric aberrationsThe correction of chromatic and geometric aberrations
Beam Delivery SystemBeam Delivery SystemBeam Delivery SystemBeam Delivery System
BDS Purpose Reduce the beam sizes to nanometer sizes to produce the BDS Purpose Reduce the beam sizes to nanometer sizes to produce the
luminosityluminosity
βx64171 m
αx-195133
βy182438 m
αy0605865
entrance
βx
7 mm
αx
0
βy
90 μm
αy
0
IP
E 15 TeV
γεx680 nm
γεy10 nm
IP
CLIC BDS OpticsCLIC BDS OpticsCLIC BDS OpticsCLIC BDS Optics
Halo and tail sourcesHalo and tail sourcesHalo and tail sourcesHalo and tail sourcesParticle processes
bull beam-gas scattering (elastic inelastic)bull Synchrotron radiation (coherentincoherent)bull Scattering off thermal photonsbull Ionelectron cloud effectsbull Intrabeam scatteringbull Touschek scattering
Optics related Halo modeling
ndash Mismatch
ndash Coupling
ndash Dispersion
ndash Non-linearities
Various (equipment related
collective)
ndash Noise and vibration
ndash Dark currents
ndash Space charge effects close to
source
ndash Wake fields
ndash Beam loading
ndash Spoiler scattering
Beam-halo collimation Beam-halo collimation Beam-halo collimation Beam-halo collimation
1048698 1048698 Beam haloBeam halo damping ring linac final focus aberrations damping ring linac final focus aberrations etcetc
1048698 1048698 The The beam halobeam halo can result in electromagnetic showers can result in electromagnetic showers and SR reaching the detector (+ muon background)and SR reaching the detector (+ muon background)
1048698 1048698 HaloHalo removed by physically intercepting the particles removed by physically intercepting the particles using mechanical spoilers + thick absorbers to remove using mechanical spoilers + thick absorbers to remove the debristhe debris
1048698 1048698 Thick absorbers then become a source of muons ndash Thick absorbers then become a source of muons ndash should be within tolerable levels at the detectorshould be within tolerable levels at the detector
1048698 1048698 IR layout and mainly final doublet dominateIR layout and mainly final doublet dominate
Beam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IP
bull Major source of detector backgroundMajor source of detector backgroundbull particles in the beam tail which hit FD andor particles in the beam tail which hit FD andor
emit photons that hit vertex detectoremit photons that hit vertex detectorbull Tails can comeTails can come
bull From FF due to aberrationsFrom FF due to aberrationsbull From damping ring linac etcFrom damping ring linac etc
bull Tails must be collimated amount of collimation Tails must be collimated amount of collimation usually determined byusually determined bybull Ratio FD bore beam size at FD Ratio FD bore beam size at FD
bull This criterion defines a maximum allowed amplitude of particles at the entrance to the FD
bull Secondary muons produced by halo interaction Secondary muons produced by halo interaction with collimators or with other aperture restriction with collimators or with other aperture restriction beamline elementsbeamline elements
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering parametersBeam-gas scattering parameters of particles = 31000 of particles = 31000 initial energy = 1496 GeV initial energy = 1496 GeV of slices = 31 of slices = 31 of macro particles = 1000 of macro particles = 1000N2 gas at room temperature (300K)N2 gas at room temperature (300K)Gas pressure = 10 nTorrGas pressure = 10 nTorr
2
2
)cos1(41
)cos1(2
1
dd el
)1log(
1
1)( mm
mel cc
cE
hcZ mincosmc
min
Angular cut-off for mott scattering cross-sectionAngular cut-off for mott scattering cross-section
Where
Angular distribution of scattered electronsAngular distribution of scattered electrons
Beam divergence
ee
Beam profile at the entranceBeam profile at the entranceBeam profile at the entranceBeam profile at the entrance
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
rad
HorizontalHorizontal
VerticalVertical
VerticalVertical
Placet-htgen simulationPlacet-htgen simulationPlacet-htgen simulationPlacet-htgen simulation
FullTrackingFullTracking
Temperature 300 KTemperature 300 K
Pressure 10 ntorrPressure 10 ntorr
Scattering angle 10 nradScattering angle 10 nrad
Residual Gas (NResidual Gas (N22))
Lattice with no collimatorsLattice with no collimators
PLACET-Development for trackingPLACET-Development for trackingHTGEN for halo generationHTGEN for halo generation
bull Total no of elements 637Total no of elements 637bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 1496 GeVLinac injection energy 1496 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nrad Emitt Along y-axis 10 nrad
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Collimation SystemCollimation System
(1) Reduce the background by removing particles at large (1) Reduce the background by removing particles at large betatron amplitudes betatron amplitudes (Halo)(Halo) or energy Offsets or energy Offsets
(2) The choice of the collimator apertures should guarantee (2) The choice of the collimator apertures should guarantee good cleaning efficiency of good cleaning efficiency of HaloHalo
(3) to avoid wakefields that might degrade the orbit stability(3) to avoid wakefields that might degrade the orbit stability
Final Focus SystemFinal Focus System
(1)(1) Need to provide a very strong focusingNeed to provide a very strong focusing(2)(2) Reduces the transverse sizes of the beam at the IP Reduces the transverse sizes of the beam at the IP
sufficiently to provide the required luminositysufficiently to provide the required luminosity(3)(3) The correction of chromatic and geometric aberrationsThe correction of chromatic and geometric aberrations
Beam Delivery SystemBeam Delivery SystemBeam Delivery SystemBeam Delivery System
BDS Purpose Reduce the beam sizes to nanometer sizes to produce the BDS Purpose Reduce the beam sizes to nanometer sizes to produce the
luminosityluminosity
βx64171 m
αx-195133
βy182438 m
αy0605865
entrance
βx
7 mm
αx
0
βy
90 μm
αy
0
IP
E 15 TeV
γεx680 nm
γεy10 nm
IP
CLIC BDS OpticsCLIC BDS OpticsCLIC BDS OpticsCLIC BDS Optics
Halo and tail sourcesHalo and tail sourcesHalo and tail sourcesHalo and tail sourcesParticle processes
bull beam-gas scattering (elastic inelastic)bull Synchrotron radiation (coherentincoherent)bull Scattering off thermal photonsbull Ionelectron cloud effectsbull Intrabeam scatteringbull Touschek scattering
Optics related Halo modeling
ndash Mismatch
ndash Coupling
ndash Dispersion
ndash Non-linearities
Various (equipment related
collective)
ndash Noise and vibration
ndash Dark currents
ndash Space charge effects close to
source
ndash Wake fields
ndash Beam loading
ndash Spoiler scattering
Beam-halo collimation Beam-halo collimation Beam-halo collimation Beam-halo collimation
1048698 1048698 Beam haloBeam halo damping ring linac final focus aberrations damping ring linac final focus aberrations etcetc
1048698 1048698 The The beam halobeam halo can result in electromagnetic showers can result in electromagnetic showers and SR reaching the detector (+ muon background)and SR reaching the detector (+ muon background)
1048698 1048698 HaloHalo removed by physically intercepting the particles removed by physically intercepting the particles using mechanical spoilers + thick absorbers to remove using mechanical spoilers + thick absorbers to remove the debristhe debris
1048698 1048698 Thick absorbers then become a source of muons ndash Thick absorbers then become a source of muons ndash should be within tolerable levels at the detectorshould be within tolerable levels at the detector
1048698 1048698 IR layout and mainly final doublet dominateIR layout and mainly final doublet dominate
Beam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IP
bull Major source of detector backgroundMajor source of detector backgroundbull particles in the beam tail which hit FD andor particles in the beam tail which hit FD andor
emit photons that hit vertex detectoremit photons that hit vertex detectorbull Tails can comeTails can come
bull From FF due to aberrationsFrom FF due to aberrationsbull From damping ring linac etcFrom damping ring linac etc
bull Tails must be collimated amount of collimation Tails must be collimated amount of collimation usually determined byusually determined bybull Ratio FD bore beam size at FD Ratio FD bore beam size at FD
bull This criterion defines a maximum allowed amplitude of particles at the entrance to the FD
bull Secondary muons produced by halo interaction Secondary muons produced by halo interaction with collimators or with other aperture restriction with collimators or with other aperture restriction beamline elementsbeamline elements
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering parametersBeam-gas scattering parameters of particles = 31000 of particles = 31000 initial energy = 1496 GeV initial energy = 1496 GeV of slices = 31 of slices = 31 of macro particles = 1000 of macro particles = 1000N2 gas at room temperature (300K)N2 gas at room temperature (300K)Gas pressure = 10 nTorrGas pressure = 10 nTorr
2
2
)cos1(41
)cos1(2
1
dd el
)1log(
1
1)( mm
mel cc
cE
hcZ mincosmc
min
Angular cut-off for mott scattering cross-sectionAngular cut-off for mott scattering cross-section
Where
Angular distribution of scattered electronsAngular distribution of scattered electrons
Beam divergence
ee
Beam profile at the entranceBeam profile at the entranceBeam profile at the entranceBeam profile at the entrance
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
rad
HorizontalHorizontal
VerticalVertical
VerticalVertical
Placet-htgen simulationPlacet-htgen simulationPlacet-htgen simulationPlacet-htgen simulation
FullTrackingFullTracking
Temperature 300 KTemperature 300 K
Pressure 10 ntorrPressure 10 ntorr
Scattering angle 10 nradScattering angle 10 nrad
Residual Gas (NResidual Gas (N22))
Lattice with no collimatorsLattice with no collimators
PLACET-Development for trackingPLACET-Development for trackingHTGEN for halo generationHTGEN for halo generation
bull Total no of elements 637Total no of elements 637bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 1496 GeVLinac injection energy 1496 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nrad Emitt Along y-axis 10 nrad
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
βx64171 m
αx-195133
βy182438 m
αy0605865
entrance
βx
7 mm
αx
0
βy
90 μm
αy
0
IP
E 15 TeV
γεx680 nm
γεy10 nm
IP
CLIC BDS OpticsCLIC BDS OpticsCLIC BDS OpticsCLIC BDS Optics
Halo and tail sourcesHalo and tail sourcesHalo and tail sourcesHalo and tail sourcesParticle processes
bull beam-gas scattering (elastic inelastic)bull Synchrotron radiation (coherentincoherent)bull Scattering off thermal photonsbull Ionelectron cloud effectsbull Intrabeam scatteringbull Touschek scattering
Optics related Halo modeling
ndash Mismatch
ndash Coupling
ndash Dispersion
ndash Non-linearities
Various (equipment related
collective)
ndash Noise and vibration
ndash Dark currents
ndash Space charge effects close to
source
ndash Wake fields
ndash Beam loading
ndash Spoiler scattering
Beam-halo collimation Beam-halo collimation Beam-halo collimation Beam-halo collimation
1048698 1048698 Beam haloBeam halo damping ring linac final focus aberrations damping ring linac final focus aberrations etcetc
1048698 1048698 The The beam halobeam halo can result in electromagnetic showers can result in electromagnetic showers and SR reaching the detector (+ muon background)and SR reaching the detector (+ muon background)
1048698 1048698 HaloHalo removed by physically intercepting the particles removed by physically intercepting the particles using mechanical spoilers + thick absorbers to remove using mechanical spoilers + thick absorbers to remove the debristhe debris
1048698 1048698 Thick absorbers then become a source of muons ndash Thick absorbers then become a source of muons ndash should be within tolerable levels at the detectorshould be within tolerable levels at the detector
1048698 1048698 IR layout and mainly final doublet dominateIR layout and mainly final doublet dominate
Beam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IP
bull Major source of detector backgroundMajor source of detector backgroundbull particles in the beam tail which hit FD andor particles in the beam tail which hit FD andor
emit photons that hit vertex detectoremit photons that hit vertex detectorbull Tails can comeTails can come
bull From FF due to aberrationsFrom FF due to aberrationsbull From damping ring linac etcFrom damping ring linac etc
bull Tails must be collimated amount of collimation Tails must be collimated amount of collimation usually determined byusually determined bybull Ratio FD bore beam size at FD Ratio FD bore beam size at FD
bull This criterion defines a maximum allowed amplitude of particles at the entrance to the FD
bull Secondary muons produced by halo interaction Secondary muons produced by halo interaction with collimators or with other aperture restriction with collimators or with other aperture restriction beamline elementsbeamline elements
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering parametersBeam-gas scattering parameters of particles = 31000 of particles = 31000 initial energy = 1496 GeV initial energy = 1496 GeV of slices = 31 of slices = 31 of macro particles = 1000 of macro particles = 1000N2 gas at room temperature (300K)N2 gas at room temperature (300K)Gas pressure = 10 nTorrGas pressure = 10 nTorr
2
2
)cos1(41
)cos1(2
1
dd el
)1log(
1
1)( mm
mel cc
cE
hcZ mincosmc
min
Angular cut-off for mott scattering cross-sectionAngular cut-off for mott scattering cross-section
Where
Angular distribution of scattered electronsAngular distribution of scattered electrons
Beam divergence
ee
Beam profile at the entranceBeam profile at the entranceBeam profile at the entranceBeam profile at the entrance
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
rad
HorizontalHorizontal
VerticalVertical
VerticalVertical
Placet-htgen simulationPlacet-htgen simulationPlacet-htgen simulationPlacet-htgen simulation
FullTrackingFullTracking
Temperature 300 KTemperature 300 K
Pressure 10 ntorrPressure 10 ntorr
Scattering angle 10 nradScattering angle 10 nrad
Residual Gas (NResidual Gas (N22))
Lattice with no collimatorsLattice with no collimators
PLACET-Development for trackingPLACET-Development for trackingHTGEN for halo generationHTGEN for halo generation
bull Total no of elements 637Total no of elements 637bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 1496 GeVLinac injection energy 1496 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nrad Emitt Along y-axis 10 nrad
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Halo and tail sourcesHalo and tail sourcesHalo and tail sourcesHalo and tail sourcesParticle processes
bull beam-gas scattering (elastic inelastic)bull Synchrotron radiation (coherentincoherent)bull Scattering off thermal photonsbull Ionelectron cloud effectsbull Intrabeam scatteringbull Touschek scattering
Optics related Halo modeling
ndash Mismatch
ndash Coupling
ndash Dispersion
ndash Non-linearities
Various (equipment related
collective)
ndash Noise and vibration
ndash Dark currents
ndash Space charge effects close to
source
ndash Wake fields
ndash Beam loading
ndash Spoiler scattering
Beam-halo collimation Beam-halo collimation Beam-halo collimation Beam-halo collimation
1048698 1048698 Beam haloBeam halo damping ring linac final focus aberrations damping ring linac final focus aberrations etcetc
1048698 1048698 The The beam halobeam halo can result in electromagnetic showers can result in electromagnetic showers and SR reaching the detector (+ muon background)and SR reaching the detector (+ muon background)
1048698 1048698 HaloHalo removed by physically intercepting the particles removed by physically intercepting the particles using mechanical spoilers + thick absorbers to remove using mechanical spoilers + thick absorbers to remove the debristhe debris
1048698 1048698 Thick absorbers then become a source of muons ndash Thick absorbers then become a source of muons ndash should be within tolerable levels at the detectorshould be within tolerable levels at the detector
1048698 1048698 IR layout and mainly final doublet dominateIR layout and mainly final doublet dominate
Beam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IP
bull Major source of detector backgroundMajor source of detector backgroundbull particles in the beam tail which hit FD andor particles in the beam tail which hit FD andor
emit photons that hit vertex detectoremit photons that hit vertex detectorbull Tails can comeTails can come
bull From FF due to aberrationsFrom FF due to aberrationsbull From damping ring linac etcFrom damping ring linac etc
bull Tails must be collimated amount of collimation Tails must be collimated amount of collimation usually determined byusually determined bybull Ratio FD bore beam size at FD Ratio FD bore beam size at FD
bull This criterion defines a maximum allowed amplitude of particles at the entrance to the FD
bull Secondary muons produced by halo interaction Secondary muons produced by halo interaction with collimators or with other aperture restriction with collimators or with other aperture restriction beamline elementsbeamline elements
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering parametersBeam-gas scattering parameters of particles = 31000 of particles = 31000 initial energy = 1496 GeV initial energy = 1496 GeV of slices = 31 of slices = 31 of macro particles = 1000 of macro particles = 1000N2 gas at room temperature (300K)N2 gas at room temperature (300K)Gas pressure = 10 nTorrGas pressure = 10 nTorr
2
2
)cos1(41
)cos1(2
1
dd el
)1log(
1
1)( mm
mel cc
cE
hcZ mincosmc
min
Angular cut-off for mott scattering cross-sectionAngular cut-off for mott scattering cross-section
Where
Angular distribution of scattered electronsAngular distribution of scattered electrons
Beam divergence
ee
Beam profile at the entranceBeam profile at the entranceBeam profile at the entranceBeam profile at the entrance
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
rad
HorizontalHorizontal
VerticalVertical
VerticalVertical
Placet-htgen simulationPlacet-htgen simulationPlacet-htgen simulationPlacet-htgen simulation
FullTrackingFullTracking
Temperature 300 KTemperature 300 K
Pressure 10 ntorrPressure 10 ntorr
Scattering angle 10 nradScattering angle 10 nrad
Residual Gas (NResidual Gas (N22))
Lattice with no collimatorsLattice with no collimators
PLACET-Development for trackingPLACET-Development for trackingHTGEN for halo generationHTGEN for halo generation
bull Total no of elements 637Total no of elements 637bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 1496 GeVLinac injection energy 1496 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nrad Emitt Along y-axis 10 nrad
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Beam-halo collimation Beam-halo collimation Beam-halo collimation Beam-halo collimation
1048698 1048698 Beam haloBeam halo damping ring linac final focus aberrations damping ring linac final focus aberrations etcetc
1048698 1048698 The The beam halobeam halo can result in electromagnetic showers can result in electromagnetic showers and SR reaching the detector (+ muon background)and SR reaching the detector (+ muon background)
1048698 1048698 HaloHalo removed by physically intercepting the particles removed by physically intercepting the particles using mechanical spoilers + thick absorbers to remove using mechanical spoilers + thick absorbers to remove the debristhe debris
1048698 1048698 Thick absorbers then become a source of muons ndash Thick absorbers then become a source of muons ndash should be within tolerable levels at the detectorshould be within tolerable levels at the detector
1048698 1048698 IR layout and mainly final doublet dominateIR layout and mainly final doublet dominate
Beam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IP
bull Major source of detector backgroundMajor source of detector backgroundbull particles in the beam tail which hit FD andor particles in the beam tail which hit FD andor
emit photons that hit vertex detectoremit photons that hit vertex detectorbull Tails can comeTails can come
bull From FF due to aberrationsFrom FF due to aberrationsbull From damping ring linac etcFrom damping ring linac etc
bull Tails must be collimated amount of collimation Tails must be collimated amount of collimation usually determined byusually determined bybull Ratio FD bore beam size at FD Ratio FD bore beam size at FD
bull This criterion defines a maximum allowed amplitude of particles at the entrance to the FD
bull Secondary muons produced by halo interaction Secondary muons produced by halo interaction with collimators or with other aperture restriction with collimators or with other aperture restriction beamline elementsbeamline elements
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering parametersBeam-gas scattering parameters of particles = 31000 of particles = 31000 initial energy = 1496 GeV initial energy = 1496 GeV of slices = 31 of slices = 31 of macro particles = 1000 of macro particles = 1000N2 gas at room temperature (300K)N2 gas at room temperature (300K)Gas pressure = 10 nTorrGas pressure = 10 nTorr
2
2
)cos1(41
)cos1(2
1
dd el
)1log(
1
1)( mm
mel cc
cE
hcZ mincosmc
min
Angular cut-off for mott scattering cross-sectionAngular cut-off for mott scattering cross-section
Where
Angular distribution of scattered electronsAngular distribution of scattered electrons
Beam divergence
ee
Beam profile at the entranceBeam profile at the entranceBeam profile at the entranceBeam profile at the entrance
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
rad
HorizontalHorizontal
VerticalVertical
VerticalVertical
Placet-htgen simulationPlacet-htgen simulationPlacet-htgen simulationPlacet-htgen simulation
FullTrackingFullTracking
Temperature 300 KTemperature 300 K
Pressure 10 ntorrPressure 10 ntorr
Scattering angle 10 nradScattering angle 10 nrad
Residual Gas (NResidual Gas (N22))
Lattice with no collimatorsLattice with no collimators
PLACET-Development for trackingPLACET-Development for trackingHTGEN for halo generationHTGEN for halo generation
bull Total no of elements 637Total no of elements 637bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 1496 GeVLinac injection energy 1496 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nrad Emitt Along y-axis 10 nrad
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Beam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IPBeam Halotail and Background at IP
bull Major source of detector backgroundMajor source of detector backgroundbull particles in the beam tail which hit FD andor particles in the beam tail which hit FD andor
emit photons that hit vertex detectoremit photons that hit vertex detectorbull Tails can comeTails can come
bull From FF due to aberrationsFrom FF due to aberrationsbull From damping ring linac etcFrom damping ring linac etc
bull Tails must be collimated amount of collimation Tails must be collimated amount of collimation usually determined byusually determined bybull Ratio FD bore beam size at FD Ratio FD bore beam size at FD
bull This criterion defines a maximum allowed amplitude of particles at the entrance to the FD
bull Secondary muons produced by halo interaction Secondary muons produced by halo interaction with collimators or with other aperture restriction with collimators or with other aperture restriction beamline elementsbeamline elements
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering parametersBeam-gas scattering parameters of particles = 31000 of particles = 31000 initial energy = 1496 GeV initial energy = 1496 GeV of slices = 31 of slices = 31 of macro particles = 1000 of macro particles = 1000N2 gas at room temperature (300K)N2 gas at room temperature (300K)Gas pressure = 10 nTorrGas pressure = 10 nTorr
2
2
)cos1(41
)cos1(2
1
dd el
)1log(
1
1)( mm
mel cc
cE
hcZ mincosmc
min
Angular cut-off for mott scattering cross-sectionAngular cut-off for mott scattering cross-section
Where
Angular distribution of scattered electronsAngular distribution of scattered electrons
Beam divergence
ee
Beam profile at the entranceBeam profile at the entranceBeam profile at the entranceBeam profile at the entrance
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
rad
HorizontalHorizontal
VerticalVertical
VerticalVertical
Placet-htgen simulationPlacet-htgen simulationPlacet-htgen simulationPlacet-htgen simulation
FullTrackingFullTracking
Temperature 300 KTemperature 300 K
Pressure 10 ntorrPressure 10 ntorr
Scattering angle 10 nradScattering angle 10 nrad
Residual Gas (NResidual Gas (N22))
Lattice with no collimatorsLattice with no collimators
PLACET-Development for trackingPLACET-Development for trackingHTGEN for halo generationHTGEN for halo generation
bull Total no of elements 637Total no of elements 637bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 1496 GeVLinac injection energy 1496 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nrad Emitt Along y-axis 10 nrad
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering Beam-gas scattering phenomenaphenomena
Beam-gas scattering parametersBeam-gas scattering parameters of particles = 31000 of particles = 31000 initial energy = 1496 GeV initial energy = 1496 GeV of slices = 31 of slices = 31 of macro particles = 1000 of macro particles = 1000N2 gas at room temperature (300K)N2 gas at room temperature (300K)Gas pressure = 10 nTorrGas pressure = 10 nTorr
2
2
)cos1(41
)cos1(2
1
dd el
)1log(
1
1)( mm
mel cc
cE
hcZ mincosmc
min
Angular cut-off for mott scattering cross-sectionAngular cut-off for mott scattering cross-section
Where
Angular distribution of scattered electronsAngular distribution of scattered electrons
Beam divergence
ee
Beam profile at the entranceBeam profile at the entranceBeam profile at the entranceBeam profile at the entrance
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
rad
HorizontalHorizontal
VerticalVertical
VerticalVertical
Placet-htgen simulationPlacet-htgen simulationPlacet-htgen simulationPlacet-htgen simulation
FullTrackingFullTracking
Temperature 300 KTemperature 300 K
Pressure 10 ntorrPressure 10 ntorr
Scattering angle 10 nradScattering angle 10 nrad
Residual Gas (NResidual Gas (N22))
Lattice with no collimatorsLattice with no collimators
PLACET-Development for trackingPLACET-Development for trackingHTGEN for halo generationHTGEN for halo generation
bull Total no of elements 637Total no of elements 637bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 1496 GeVLinac injection energy 1496 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nrad Emitt Along y-axis 10 nrad
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Beam profile at the entranceBeam profile at the entranceBeam profile at the entranceBeam profile at the entrance
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
rad
HorizontalHorizontal
VerticalVertical
VerticalVertical
Placet-htgen simulationPlacet-htgen simulationPlacet-htgen simulationPlacet-htgen simulation
FullTrackingFullTracking
Temperature 300 KTemperature 300 K
Pressure 10 ntorrPressure 10 ntorr
Scattering angle 10 nradScattering angle 10 nrad
Residual Gas (NResidual Gas (N22))
Lattice with no collimatorsLattice with no collimators
PLACET-Development for trackingPLACET-Development for trackingHTGEN for halo generationHTGEN for halo generation
bull Total no of elements 637Total no of elements 637bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 1496 GeVLinac injection energy 1496 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nrad Emitt Along y-axis 10 nrad
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole Beam profile in the final quadrupole
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Hori
zon
tal an
gle
Hori
zon
tal an
gle
Vert
ical an
gle
Vert
ical an
gle
VerticalVertical
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
rad
HorizontalHorizontal
VerticalVertical
VerticalVertical
Placet-htgen simulationPlacet-htgen simulationPlacet-htgen simulationPlacet-htgen simulation
FullTrackingFullTracking
Temperature 300 KTemperature 300 K
Pressure 10 ntorrPressure 10 ntorr
Scattering angle 10 nradScattering angle 10 nrad
Residual Gas (NResidual Gas (N22))
Lattice with no collimatorsLattice with no collimators
PLACET-Development for trackingPLACET-Development for trackingHTGEN for halo generationHTGEN for halo generation
bull Total no of elements 637Total no of elements 637bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 1496 GeVLinac injection energy 1496 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nrad Emitt Along y-axis 10 nrad
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
Halo Phase space plots in final Halo Phase space plots in final quadrupolequadrupole
rad
HorizontalHorizontal
VerticalVertical
VerticalVertical
Placet-htgen simulationPlacet-htgen simulationPlacet-htgen simulationPlacet-htgen simulation
FullTrackingFullTracking
Temperature 300 KTemperature 300 K
Pressure 10 ntorrPressure 10 ntorr
Scattering angle 10 nradScattering angle 10 nrad
Residual Gas (NResidual Gas (N22))
Lattice with no collimatorsLattice with no collimators
PLACET-Development for trackingPLACET-Development for trackingHTGEN for halo generationHTGEN for halo generation
bull Total no of elements 637Total no of elements 637bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 1496 GeVLinac injection energy 1496 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nrad Emitt Along y-axis 10 nrad
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Placet-htgen simulationPlacet-htgen simulationPlacet-htgen simulationPlacet-htgen simulation
FullTrackingFullTracking
Temperature 300 KTemperature 300 K
Pressure 10 ntorrPressure 10 ntorr
Scattering angle 10 nradScattering angle 10 nrad
Residual Gas (NResidual Gas (N22))
Lattice with no collimatorsLattice with no collimators
PLACET-Development for trackingPLACET-Development for trackingHTGEN for halo generationHTGEN for halo generation
bull Total no of elements 637Total no of elements 637bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 1496 GeVLinac injection energy 1496 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nrad Emitt Along y-axis 10 nrad
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Beam coreBeam core
Beam-HaloBeam-Halo
Collimations region Final Focus
Halomdashparticles with large Halomdashparticles with large
betatron amplitudes or with betatron amplitudes or with
large energy off-setslarge energy off-sets
Longitudinal coordinateLongitudinal coordinate
Beam Delivery SystemBeam Delivery System
Beam squeezing leads
the vertical dispersion
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)Beam-Halo (Residual Gas pressure dependence)
84 gt1mm
17 gt 10mm
53 gt1mm
05 gt 10mm
82 gt1mm
04 gt 10mm
No significant change in vertical halo (above 1mm) as we go from 1-10 ntorrNo significant change in vertical halo (above 1mm) as we go from 1-10 ntorr
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)Beam-Halo (scattering angle dependence)
03 gt1mm)03 gt1mm)
0004 gt10mm 0004 gt10mm
62 gt1mm62 gt1mm
04 gt 10mm04 gt 10mm
84 gt1mm84 gt1mm
17 gt 10mm17 gt 10mm
Small angle less
vertical expension
Inverse of above
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Halo- energy dependenceHalo- energy dependenceHalo- energy dependenceHalo- energy dependence
Low energy beamLow energy beam
bullLarge energy spread (~1Large energy spread (~1
bullLarge vertical off-setLarge vertical off-set
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Halo gt 102m = 30
Halo gt 1 mm = ~ 3
Halo gt 10 mm = ~ 05
Beam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with apertureBeam and Halo Profile with aperture
1031
Lattice provided by Javier Resta-lopez
octupole octupole
collimatorcollimator
++
spoilersspoilers
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Scatt angleScatt angle Gas pressureGas pressure of halo of halo of lost of lost Lost Lost probabilityprobability
File sizeFile size
q = 01q = 01 10 ntorr10 ntorr ~ 132572~ 132572 55 37x1037x10-5-5 13 MB13 MB
q = 001q = 001 1 ntorr1 ntorr ~ 132572~ 132572 00 13 MB13 MB
q = 001q = 001 5 ntorr5 ntorr ~ 8176465~ 8176465 00 796 MB796 MB
q = 001q = 001 10 ntorr10 ntorr ~ 8176465~ 8176465 22 24x1024x10-7-7 796 MB796 MB
q = 0008q = 0008 10 ntorr10 ntorr ~ 20036933~ 20036933 55 25x1025x10-7-7 2 GB2 GB
Electron beam = 1972236 (192 MB)Electron beam = 1972236 (192 MB) lattice V-06-09-01lattice V-06-09-01
halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 10nt 8176465 ratio 10nt5nt==128 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 5nt 6382848 ratio 5nt1nt== 5 halo at angle = 001 P = 1nt 1282543 halo at angle = 001 P = 1nt 1282543 (63 times 1---gt 10 ntorr pressure)(63 times 1---gt 10 ntorr pressure)
---------------------------------------------------------------------------------------------------------------------------------------- halo at angle = 01 P = 10nt 132572 halo at angle = 01 P = 10nt 132572 halo at angle = 005 P = 10nt 531363 halo at angle = 005 P = 10nt 531363 halo at angle = 001 P = 10nt 20036933 halo at angle = 001 P = 10nt 20036933 (150 times 01 (150 times 01 rad---gt rad---gt rad )rad )
Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)Halo Statistics (BDS)
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Halo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINACHalo Distributions in LINAC
bull FullTrackingFullTrackingbull Temperature 300 KTemperature 300 Kbull Pressure 10 ntorrPressure 10 ntorrbull Scattering angle 10nradScattering angle 10nradbull Residual GasResidual Gas
bull Standard PLACET latticeStandard PLACET latticebull Total no of elements 54068Total no of elements 54068
bull No of Quad 1324No of Quad 1324bull No of BPMs 1324No of BPMs 1324
bull No of slices 31No of slices 31bull No of macroparticles 100No of macroparticles 100bull Linac injection energy 90 GeVLinac injection energy 90 GeVbull Charge 4 nCCharge 4 nCbull Emitt along x-axis 680 nradEmitt along x-axis 680 nradbull Emitt Along y-axis 10 nradEmitt Along y-axis 10 nrad
LINAC Beamline LINAC Beamline
Energy of the halo particles is increasing Energy of the halo particles is increasing
almost linearly during passing through the almost linearly during passing through the
acceleratoing structures of the LINACacceleratoing structures of the LINAC
PLACET-HTGEN TrackingPLACET-HTGEN Tracking
Several problems pointed out by me and then
fixed immediately by Helmut
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Halo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINACHalo spectrum in LINAC
HorizontalHorizontal
VerticalVertical
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Found no loss of halo Found no loss of halo
Beam-gas scattering + Beam-gas scattering +
Bremsstraulung both Bremsstraulung both
processes are contributing processes are contributing
here due to low energy beam here due to low energy beam
at the time of injectionat the time of injection
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Halo in Post collision lineHalo in Post collision lineHalo in Post collision lineHalo in Post collision line
Halo and beam looks same so halo are Halo and beam looks same so halo are
not so important for extraction line but not so important for extraction line but
beam distributions countbeam distributions count
PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP PLACET-HTGEN Tracking input from GUINEA-PIG (Beam-Beam effects at IP
soon will be presented)soon will be presented)
Lattice used contains only driftsLattice used contains only drifts
With no collimatorsWith no collimators
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
PLA
CET v
s D
IMA
D
PLA
CET v
s D
IMA
D (A
rnau
d f
era
ri)
(Arn
au
d f
era
ri)
Horizontal phase spaceVertical phase space
o
f entr
ies
o
f entr
ies
o
f entr
ies
o
f entr
ies
HorizontalHorizontalVerticalVertical
HorizontalHorizontal
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Summary Summary Halo estimates and simulationsHalo estimates and simulationsSummary Summary Halo estimates and simulationsHalo estimates and simulations
by H Burkhardt L Neukermans1 A Latina I Ahmed CERN
Done 2007 bull htgen software package with installation instructions interfaces to tracking codes and examples made availablebull htgen provides simulation and estimates of main halo production processes applied to ILC amp CLIC
Process availablebull Beam-gas elastic scattering (mott)bull Beam-gas in-elastic scattering (Bremsstrahlung)
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
SummarySummarySummarySummary
Ongoing and future work Ongoing and future work
bull Online manual for the htgen software packageOnline manual for the htgen software packagebull Improve the HTGEN package Improve the HTGEN package bull Simplify HTGEN commands and provide control and Simplify HTGEN commands and provide control and
diagnostics output implement further halo production diagnostics output implement further halo production mechanismsmechanisms
bull Reduce dependence on external libs (CLHEP GS in Reduce dependence on external libs (CLHEP GS in case of placet) cleaner interfaces -- less globals and case of placet) cleaner interfaces -- less globals and copying of structurescopying of structures
bull Update to recent synchrotron radiation code work with Update to recent synchrotron radiation code work with HTGEN users provide help and follow up on requests HTGEN users provide help and follow up on requests tests and benchmarking measurements (ATF CTF3) tests and benchmarking measurements (ATF CTF3) and with other codes -- Geant4 BDSIMand with other codes -- Geant4 BDSIM
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Objectives and upcomingObjectives and upcomingObjectives and upcomingObjectives and upcoming
Halo estimation in Drive beam system Halo estimation in Drive beam system (struggling but PETS--)(struggling but PETS--)
Halo estimation in Beam Delivery System Halo estimation in Beam Delivery System (Done)(Done)
Halo estimation in Post-collision line Halo estimation in Post-collision line (Done even not so important)(Done even not so important)
Halo estimation in Main LINACHalo estimation in Main LINAC(Done)(Done)
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
Back-up SlidesBack-up SlidesBack-up SlidesBack-up Slides
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-
- Slide 1
- Beam Delivery System
- CLIC BDS Optics
- Halo and tail sources
- Beam-halo collimation
- Beam Halotail and Background at IP
- Beam-gas scattering phenomena
- Beam profile at the entrance
- Beam profile in the final quadrupole
- Halo Phase space plots in final quadrupole
- Placet-htgen simulation
- Slide 12
- Slide 13
- Beam-Halo (scattering angle dependence)
- Halo- energy dependence
- Slide 16
- Slide 17
- Halo Distributions in LINAC
- Halo spectrum in LINAC
- Slide 20
- Halo in Post collision line
- Slide 22
- Summary Halo estimates and simulations
- Summary
- Objectives and upcoming
- Back-up Slides
- Slide 27
-