1 clic*lhc based fel*nucleus collider clic*lhc based fel*nucleus collider o. yavas 1 with the...

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1 CLIC*LHC CLIC*LHC Based Based FEL*Nucleus FEL*Nucleus Collider Collider O. Y O. Y avas avas 1 with the contributions of R. Corsini with the contributions of R. Corsini 2 E. Guliyev E. Guliyev 1,3 1,3 , , A. A. Özcan Özcan 4 S. Sultansoy S. Sultansoy 3,4 3,4 , S , S . Yigit . Yigit 1,5 1,5 1 Ankara Ankara U niversity, Ankara niversity, Ankara 2 CERN CERN 3 Acad. of Sciences, Baku Acad. of Sciences, Baku 4 Gazi University, Ankara Gazi University, Ankara 5 TAEK, TAEK, Ankara Ankara MINIWORKSHOP ON MACHINE AND PHYSICS ASPECTS OF CLIC BASED FUTURE COLLIDERS August 30, 2004 CERN

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Page 1: 1 CLIC*LHC Based FEL*Nucleus Collider CLIC*LHC Based FEL*Nucleus Collider O. Yavas 1 with the contributions of R. Corsini 2 E. Guliyev 1,3, A. Özcan 4

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CLIC*LHCCLIC*LHC BasedBasedFEL*NucleusFEL*Nucleus ColliderCollider

O. YO. Yavasavas11

with the contributions of R. Corsiniwith the contributions of R. Corsini22 E. GuliyevE. Guliyev1,31,3, , A. A. ÖzcanÖzcan44 S. SultansoyS. Sultansoy3,43,4, S, S. Yigit. Yigit1,5 1,5

11Ankara Ankara UUniversity, Ankara niversity, Ankara 22CERNCERN

33Acad. of Sciences, BakuAcad. of Sciences, Baku44Gazi University, Ankara Gazi University, Ankara

55TAEK,TAEK, AnkaraAnkara

MINIWORKSHOP ON MACHINE AND PHYSICS ASPECTS OFCLIC BASED FUTURE COLLIDERS August 30, 2004 CERN

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MotivationMotivation

In principle, a FEL beam can be used forIn principle, a FEL beam can be used for thethe excitations of any fully ioni excitations of any fully ionizzed ed relativistic nucleus beam relativistic nucleus beam to study to study

Nuclear Spectroscopy...Nuclear Spectroscopy...

In In such a FEL-Nucleus collider;such a FEL-Nucleus collider;

The accelerated fully ioniThe accelerated fully ionized zed nuclei will “nuclei will “seesee” the keV energy photons as a ” the keV energy photons as a MeV energy laser beam.MeV energy laser beam.

H. Aktas et al.H. Aktas et al. New tool for ‘old’ nuclear physics: FEL-Nucleus CollidersNew tool for ‘old’ nuclear physics: FEL-Nucleus Colliders

Nuc. Instr. &Nuc. Instr. & Meth A428 (1999)Meth A428 (1999) 271-275271-275

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FEL*Nucleus ColliderFEL*Nucleus Collider

The main advantages compared to the traditional The main advantages compared to the traditional NRF NRF methods are tunability, methods are tunability, monochromaticity and high polarization of monochromaticity and high polarization of FEL beam. FEL beam.

The advantages result in higher statistic and the possibility to investigate The advantages result in higher statistic and the possibility to investigate individual levels.individual levels.

General schematic view of theGeneral schematic view of the proposed designproposed design

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FEL*Nucleus ColliderFEL*Nucleus Collider

The energy of FEL photons needed for excitation at the corresponding nuclei level can be expressed as

Due to good monochromaticity Due to good monochromaticity ((EE/E/E <10<10-3-31010-4-4)) with the typical obtainable with the typical obtainable number of photons number of photons ((101013 13 /bunch/bunch) ) and excellent tunability, this method can be and excellent tunability, this method can be successfully used to investigate nuclear excitations with low multipolarity successfully used to investigate nuclear excitations with low multipolarity (E1 and (E1 and M1) M1) in wide energy region.in wide energy region.

Especially, collective excitations of nuclei can be analyze in detail using the Especially, collective excitations of nuclei can be analyze in detail using the monochromaticity of FEL beam.monochromaticity of FEL beam.

N p

Z

A p=7462 for LHC

p

exc

N

excFEL

E

Z

AE

22

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CLIC*LHC Based FEL-Nucleus ColliderCLIC*LHC Based FEL-Nucleus Collider

FEL beam can be obtained from CLIC FEL beam can be obtained from CLIC drive drive beam..beam....

Nucleus beams from LHCNucleus beams from LHC ......

CLIC*LHC Based FEL*Nucleus Collider !CLIC*LHC Based FEL*Nucleus Collider !

This collider allows to study Nuclear Spectroscopy precisely This collider allows to study Nuclear Spectroscopy precisely using tunable, monochromatic and coherent radiation FEL using tunable, monochromatic and coherent radiation FEL from CLIC which collide with LHC Nucleus beams (Pb, C, Sm, from CLIC which collide with LHC Nucleus beams (Pb, C, Sm, Au, Ce, Ba etc.)Au, Ce, Ba etc.)

Luminosity: Luminosity:

Event rate: Event rate:

4nuc

cx y

n nL f

aveR L

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An ideal photon source used in (An ideal photon source used in (,,’) scattering ’) scattering experiments should have the following experiments should have the following

characteristicscharacteristics**

- High spectral intensity High spectral intensity ( (I=NI=N /eV s/eV s))

- Good monochromaticity Good monochromaticity ( (EE/E/E))

- Tunable in a broad energy rangeTunable in a broad energy range (IR - Hard X-ray) (IR - Hard X-ray)

- High degree of linear polarizationHigh degree of linear polarization ( (PP=100%)=100%)

**U.Kneissl et al. Prog.Part.Nucl. Phys. 37 (1996) 349U.Kneissl et al. Prog.Part.Nucl. Phys. 37 (1996) 349

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Characteristics of the different photon sourcesCharacteristics of the different photon sources

Photon SourcePhoton Source SpeSpecctral tral IntensitIntensityy [[/s·eV]/s·eV]

EE/E/E

[%][%]PP [%] [%] Target Target

Mass Mass

M M [g][g]

CCompton ompton Backscattered Backscattered

BBremsstrahlungremsstrahlung

(Polarised)(Polarised)

..BBremsstrahlung remsstrahlung

(Unpolarised) + CB(Unpolarised) + CB

BBremsstrahlungremsstrahlung

(Unpolarised)(Unpolarised)

Free Free EElectron lectron LLaseraser

0.150.15

2020

10001000

10001000

10101717 MeV/E MeV/Eexcexc

2.72.7

Cont.Cont.

Cont.Cont.

Cont.Cont.

0.010.01

100100

10-3010-30

10-2010-20

00

100100

7070

55

55

1-21-2

1010-10-10

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Nuclear Resonant FlouresanceNuclear Resonant Flouresance (NRF) Methods(NRF) Methods

The observables which can be obtained from NRF are*:The observables which can be obtained from NRF are*:

- The energy of the state - The energy of the state - The - The -decay branching ratios to the ground state and excited states,-decay branching ratios to the ground state and excited states,- The multipolarity of the tranThe multipolarity of the transsition and theition and the spin spin of excited of excited states,states,- The absolute transition strength or lifetime of the state if all decayThe absolute transition strength or lifetime of the state if all decay branches are known,branches are known,- - TThe parihe paritty of the state.y of the state.____________________________________________________**All these observables are independent from nuclear modelAll these observables are independent from nuclear model

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TThe experimental capacity of NRF methods are he experimental capacity of NRF methods are limited by many factorslimited by many factors

- - While the used photons energy increasing While the used photons energy increasing (> 4 MeV)(> 4 MeV) the polarization of the polarization of photons are decreases. photons are decreases.

- TThe rather weak interaction between the photons and the target material.he rather weak interaction between the photons and the target material. Therefore, one needs for typical obtainable photon currents of aboutTherefore, one needs for typical obtainable photon currents of about

101066 /(s keV)/(s keV) at the target position large amounts of isotopically enriched at the target position large amounts of isotopically enriched target material target material (i.e. around(i.e. around 500 mg 500 mg))

- Very long experiment time: For the 4-8 MeV spectra, the typical - Very long experiment time: For the 4-8 MeV spectra, the typical count rates in the Ge (HP) detectorscount rates in the Ge (HP) detectors are in order of a few thousands are in order of a few thousands perper secondsecond leadingleading to typical measuring times of several hours. to typical measuring times of several hours.

- - HHigh energy background irradiation fromigh energy background irradiation from evidence materialevidence material

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Energy RangesEnergy Ranges

Energy range for E1 and M1 dipole excitations : Energy range for E1 and M1 dipole excitations :

EEexc exc = 2-20 MeV = 2-20 MeV

Energy of nucleus beam of LHC: Energy of nucleus beam of LHC:

EEAA== m mA A cc2 , 2 , pp , , p p ~ 7~ 7464622

Needed FEL energies: Needed FEL energies:

FEL FEL = 0.3 – 3 keV (for LHC nucleus beams)= 0.3 – 3 keV (for LHC nucleus beams)

(4(4 –– 0. 0.4 nm) E4 nm) Eexcexc = 2 = 2 FELFEL

Needed electron beam energies from CLICNeeded electron beam energies from CLIC

EEelectron electron = 1 – = 1 – 44 GeV GeV

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Basic Requirements for SASE FEL BeamBasic Requirements for SASE FEL Beam

Ee/Ee ~ ~ 10-3 FEL Parameter)

Normalized emittance

Gain Length

FEL Gain Parameter:

Power saturation:

4

l ug

4/, yx

uNG 4

beamsat PP

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CLIC*LHC based FEL-nucleus collider

Advantages of CLIC FEL:

• Compact linac• Existing equipment (if CLIC is built)

Disadvantages of CLIC FEL:

• High-frequency RF large energy spread (short range wakes)

• Normal conducting difficult to match time structure of nucleus beam

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CLIC*LHC based FEL-nucleus collider

Possible solution:

Don’t use CLIC main beam (energy too high after damping ring, emittance too large before, large energy spread …)

Use additional drive beam pulses to power a dedicated linac -

15 GHz could be used, in order to obtain a smaller energy spread

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Red point corresponds to drive beam with 15 GHz acceleration

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FEL & e- beam parameters

•Photon (FEL) energies: 0.3-3.4 keV = 4 - 0.4 nm

•Electron beam energies: Eb = 1 - 4 GeV

•Wiggler W= 2.3 cm, BW = 0.38 T, aW = 0.8

•Qb = 1 nC, p/p ~ 10-3 , norm,rms ~ 2 10-6, lbunch = 50 m

•Photon beam size (transverse) < 50 m

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FEL & e- beam parameters

Need dedicated source (photoinjector), staged bunch compressor

Assuming 15 GHz, 60 MV/m gradient & fill factor 0.75: linac length < 70 m wiggler length < 20 m

Time structure:

“minimum” scenario: single bunch, 100 Hz rep rate:

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Luminosity (Single Bunch Scenario)

L= 1.87 ·1027

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100 ns

250 ps rms

Ion beam (Pb)

592 bunches

•Use drive beam pulses after delay loop•Use 50 ns long sub-pulses, 100 ns between pulses (special delay loop ?)•Can cover 10 ion bunches every 1s additional DB pulse length

Drive Beam “Double pulse” scheme

(new parameter set*)

From DBA – 56 ns long “sub-pulses”

After delay loop - combination four by four in 2 batches in 1st combiner ring

After 1st combiner ring - combination four by four in 2 batches in 2nd combiner ring

56 ns

~ 1 s

Time structure matching

* http://clic-meeting.web.cern.ch/clic-meeting/par-table.html

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Multi-pulse scenario, 100 Hz rep rate:

Matched transverse beam

size

For 5 s drive beam pulse(about 5 % of CLIC total power consumption)

L = 4.4 1029

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Power balance, accelerating structures parameters:

Take 1.8 GeV drive beam9 A drive beam currentTotal power in DB: 16 GWAssume total transfer DB to RF ~ 75 %Get ~ 12 GW

Assume 60 MV/m active length 50 m - Available 240 MW/m

Example structures:

NLC 11.4 GHz 50-65 MV/m for 75 MW input, 0.9 m long

fill time 120 ns

SICA (CTF3) 3 GHz ~ 14 MV/m for 30 MW input, 1 m longfill time 100 ns

Scaling SICA at 15 GHz, one would get about 0.6 m length for 50 ns fill time, and 60 MW input power for a gradient of 60 MV/m

Would need only about 110 MW/m – large margin (but low power extraction efficiency from the drive beam) – the available power would be enough to drive the structures at about 90 MV/m

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Main Parameters of LHC Pb BeamMain Parameters of LHC Pb Beam

Energy per nucleon (TeV/u) 2.76Energy per nucleon (TeV/u) 2.76 # of ions per bunch (10# of ions per bunch (1077) 7) 7 # of bunches 592# of bunches 592 Bunch seperation (ns) 99.8Bunch seperation (ns) 99.8 Transverse beam size (Transverse beam size (m) 15.9m) 15.9

Luminosity for Pb-Pb coll. (cmLuminosity for Pb-Pb coll. (cm-2-2ss-1-1) 10) 102727 (ALICE Exp.)(ALICE Exp.) Energy ranges for FEL*Pb CollisionsEnergy ranges for FEL*Pb Collisions

;2.1 GeVEe MeVEexc 2.

;4 GeVEe MeVEexc 20.

;34.0 keVFEL

;4.3 keVFEL

2941,2 PbFELPbexcE

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Process Example for Process Example for 208208PbPb The cross section for the resonant photon scattering is given by the well-known The cross section for the resonant photon scattering is given by the well-known Breit –Wigner formulaBreit –Wigner formula

Where E is the c.m. energy of the incoming photon, JWhere E is the c.m. energy of the incoming photon, Jexc exc and Jand J0 0 are spins of the excited are spins of the excited and gorund states of the nucleus, Eand gorund states of the nucleus, ERR is the energy at the resonance and is the energy at the resonance and is the total is the total width of the excited nucleus. The number of the scattering events from the nuclei of width of the excited nucleus. The number of the scattering events from the nuclei of 208208PbPb has roughly been calculated below taking their excited state of has roughly been calculated below taking their excited state of 4842.24842.2 keV keV respectively. One can easily obtain corresponding values for other excitations and respectively. One can easily obtain corresponding values for other excitations and other nuclei. other nuclei.

In this case In this case 00= 808 eV= 808 eV and and EEee=2.05=2.05 GeVGeV. Substituting J. Substituting Jexcexc=1, J=1, J00=0, =0, 5 eV. Using 5 eV. Using these value resonant cross section has been estimated asthese value resonant cross section has been estimated as

and, consequently, with the same energy spreads given above, the average cross and, consequently, with the same energy spreads given above, the average cross section assection as

Which corresponds to Which corresponds to 2.1x102.1x1088 events per day for events per day for L= 4.4 10L= 4.4 102929 cm cm-2-2 s s-1-1

4/)()12(2

12`),(

22

2

02

R

exc

EEJ

J

E

222101.3 cmres

224103.0 cmav

Eresav

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E MeV (eV) J FEL, keV res cm2 ave cm2 R/s

4.0852 7.8310-1 2+ 0.694 7.310-22 1.3910-24 6.1105

4.8422 99.7210-1 1- 0.823 5.2310-22 1.0710-23 4.7106

5.2926 13.16100 1- 0.899 2.6210-22 2.6210-24 2.8106

5.5122 32.91100 1- 0.937 2.4110-22 0.1410-22 6.1107

5.8461 11.5410-1 1+ 0.993 21.510-22 4.2510-24 1.8105

5.9480 10.1210-1 1- 1.011 2.0710-22 3.5210-25 1.5104

6.2640 10.1210-1 1- 1.064 1.8710-22 3.0210-25 1.3104

6.3117 36.5610-1 1- 1.072 1.0610-22 1.0610-24 4.6105

6.3628 10.4410-1 1- 1.081 1.8110-22 2.9610-25 1.3104

6.7205 10.97100 1- 1.142 1.6210-22 2.6410-24 1.1105

6.9800 50.6410-1 - 1.186 - - -

7.0635 28.61100 1- 1.200 1.4710-22 5.9510-24 2.6105

7.0834 14.62100 1- 1.200 1.4610-22 3.6210-24 1.5105

7.2430 15.6710-1 - 1.231 - - -

7.2780 15.6710-1 - 1.237 - - -

7.2789 14.0010-1 1+ 1.237 1.3810-22 2.6510-25 1.1104

7.3325 38.7110-0 1- 1.246 1.3610-22 7.1810-24 3.1105

7.6853 - - 1.306 - - -

10.050 - - 1.708 - - -

10.600 - - 1.801 - - -

11.450 - - 1.975 - - -

),( scattering results for excitations of 208Pb

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FEL-LHC (FEL-LHC (154154Sm example)Sm example)

EExisting (xisting (,,`) facilities are not suitable for investigation of `) facilities are not suitable for investigation of excitations with Eexcitations with Eexcexc > 5 MeV. On the other hand, theoretical models > 5 MeV. On the other hand, theoretical models

predicts a lot of levels in this region. Therefore here we present predicts a lot of levels in this region. Therefore here we present results obtained from experiment and from microscopic model used results obtained from experiment and from microscopic model used RPA approximation. RPA approximation.

We studied the main parameters of FEL-LHC (Sm) collider We studied the main parameters of FEL-LHC (Sm) collider considering TTF FEL like photon beam and obtained 10considering TTF FEL like photon beam and obtained 103030 cm cm-2-2ss-1-1 luminosity (E. Guliyev et al. 2002). Following tables show the luminosity (E. Guliyev et al. 2002). Following tables show the needed FEL energies, spin and parities of states and event rates.needed FEL energies, spin and parities of states and event rates.

Following first table show the results for experimentaly observed Following first table show the results for experimentaly observed states ( Estates ( Eexcexc< 3.844). It is clear that spin and parity values of some < 3.844). It is clear that spin and parity values of some

levels had not determined with NRF experiments. Results for the levels had not determined with NRF experiments. Results for the only theoretically predicted levels can be seen in second table for only theoretically predicted levels can be seen in second table for the Ethe Eexcexc > 5.155 MeV. > 5.155 MeV.

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Detector DistancesDetector DistancesThe excited nucleus will turn to the The excited nucleus will turn to the

ground state at a distanceground state at a distance

As an example, for two levels of any As an example, for two levels of any nucleus we can obtained (probably for nucleus we can obtained (probably for low and high decay widths) following low and high decay widths) following value:value:

;cl NN

;4meV ml 36.0

;2 eV ml 71036.7

1610582.6

N

As a result, one can say that for the detector size and position we have no any hardness.

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Measure of unknown decay widthMeasure of unknown decay widthFEL Nucleus collider will give opportunity to measure unknown decay widthusing known ones. Indeed, decay width can be estimated using following relation*

Where index 1 (2) correspond to level with unknown (known) decay width.For N(1) we can use 100 events per second as the observation limit.

Eresav

As an example, if we use 4.085 MeV level, =0.783 eV, res=7.3 10-22

and N(2)= 6.1 105 events/s, the upper limit for decay width of 11.45 MeV level (res = 0.5 10-22 , J=1) is determined as 5.24 10-3 eV using 100 events per second as the observation limit.

*H.Koru et al. Int. J. of Mod. Phys. 12 (2003) 533.

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Determination of spin of stateDetermination of spin of state

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Normalized energy distributions of photons emitted by spin 1 (dashed curve) and spin 2 (continuous curve) excitations of the nucleus (Th example)

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Feasibility of such a collider needs more Feasibility of such a collider needs more R&D on…R&D on…

Bunch and pulse structures of electron, FEL and Bunch and pulse structures of electron, FEL and nucleus beams…nucleus beams…

SASE FEL optimization…SASE FEL optimization… Luminosity optimization…Luminosity optimization… Open problems of nuclear spectroscopy…Open problems of nuclear spectroscopy… Ion program of LHCIon program of LHC ( (Pb, Ce, Sm, Ba, C etc.)Pb, Ce, Sm, Ba, C etc.)...... Detector design for scattered high energy photons…Detector design for scattered high energy photons…

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ReferencesReferences H. Aktas, N. Buget, A.K. Ciftci, N. Meric, S. Sultansoy, O. YavasH. Aktas, N. Buget, A.K. Ciftci, N. Meric, S. Sultansoy, O. Yavas New tool for ‘old’ nuclear physics: FEL-Nucleus CollidersNew tool for ‘old’ nuclear physics: FEL-Nucleus Colliders Nuc. Instr. &Nuc. Instr. & Meth A428 (1999)Meth A428 (1999) 271-275271-275

E.Guliyev, O. Yavas, S. SultansoyE.Guliyev, O. Yavas, S. Sultansoy Collective excitations of the 154sm nucleus at theCollective excitations of the 154sm nucleus at the FEL*LHC FEL*LHC ccolliderollider Int. J. Int. J. oof mod. Phys. E11 (2002) 501-508f mod. Phys. E11 (2002) 501-508

H. Koru, A. Ozcan, S. Sultansoy, O. YavasH. Koru, A. Ozcan, S. Sultansoy, O. Yavas Physics potential of the e-RHIC based FEL- nucleus (Th) Physics potential of the e-RHIC based FEL- nucleus (Th) ccolliderollider Int. J. Int. J. oof mod. Phys. E12 (2003) 533-542 f mod. Phys. E12 (2003) 533-542

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