ion beam collimation for the fair synchrotron sis100 · 2019. 2. 28. · beam ) beam pipe primary...

1
10 -3 10 -2 10 -1 10 0 Impact parameter [ μm] 10 -1 10 0 10 1 10 2 Fraction of particles hit PC [ %] 12 C 18+ 40 Ar 18+ 84 Kr 36+ 132 Xe 54+ 10 -3 10 -2 10 -1 10 0 Impact parameter [ μm] 70 75 80 85 90 95 100 Collimation efficiency [ %] 12 C 18+ 40 Ar 18+ 84 Kr 36+ 132 Xe 54+ Beam ) Beam pipe Primary collimator 1. secondary collimator 2. secondary collimator Beam pipe Beam Halo 10 -3 10 -2 10 -1 10 0 Impact parameter δ [μm] 10 -7 10 -6 10 -5 10 -4 10 -3 10 -2 10 -1 10 0 -δ p/p 1 H 1+ 2 H 1+ 4 He 2+ 12 C 6+ 14 N 7+ 16 O 8+ 20 Ne 10+ 40 Ar 18+ 84 Kr 36+ 132 Xe 54+ 181 Ta 73+ 197 Au 79+ 1 H 2 H 4 He 12 C 14 N 16 O 20 Ne 40 Ar 84 Kr 132 Xe 181 Ta 197 Au 50 60 70 80 90 100 Collimation efficiency [%] multi pass efficiency single pass efficiency 10 -3 10 -2 10 -1 10 0 Impact parameter δ [μm] 10 -2 10 -1 10 0 10 1 x,r.m.s. [mrad] 1 H 1+ 2 H 1+ 4 He 2+ 12 C 6+ 14 N 7+ 16 O 8+ 20 Ne 10+ 40 Ar 18+ 84 Kr 36+ 132 Xe 54+ 181 Ta 73+ 197 Au 79+ 0 5 10 15 s [m] -75 -50 -25 0 25 50 75 x [mm] PC 1.SC QF QD 2.SC 47.7% lost in 1.SC 23.7% lost in 2.SC 0.0% lost in Quad 28.6% escaped Beam envelope 4.5σ Abstract *[email protected] This work is supported by BMBF contract 05P12RDRBM Ion Beam Collimation for the FAIR Synchrotron SIS100 Ivan Prokhorov * TEMF, TU Darmstadt, Darmstadt, Germany Ivan Strasik and Oliver Boine-Frankenheim GSI, Darmstadt, Germany The collimation system for the SIS 100 synchrotron has to operate with protons as well as with light and heavy fully-stripped ions ( 2 H 1+ - 197 Au 79+ ). The concept and basic design features of the betatron halo collimation in SIS 100 were developed previously for proton operation. The main task of the presented work is to compare the efficiency of proton and ion beam collimation. For this purpose multi pass tracking of halo particles was performed using MAD-X including the simulation of scattering process and energy loss in the collimators using the ATIMA code. The collimation efficiency as a function of the ion species together with the detailed beam loss distribution along the ring circumference are presented. θ r . m . s = 13.6 MeV βpc Z x X 0 1+ 0.38ln x X 0 ( ) Motivation Beam halo is non-Gaussian tails of a beam. It occurs due to beam dynamics aspects (beam instabilities, IBS, beam mismatch) and machine imperfections (RF noises, magnet errors and misalignments). Principles of collimation 1. J.B. Jeanneret, Phys. Rev. ST Accel. Beams 1 (1998) 081001 2. P. Spiller et al., “Status of the SIS 100 heavy ion synchrotron project at FAIR”, IPAC’13, Shanghai, May 2013, THPWO011. 3. http://web-docs.gsi.de/~weick/atima/ 4. A.H. Soerensen J. Lindenhard. Relativistic theory of stopping for heavy ions. Phys. Rev., A53:2443, 1996. 5. http://mad.web.cern.ch/ Collimators in SIS 100 CERN Accelerator School: Accelerator Physics Advanced Level Trondheim, Norway 24 August 2013 The two-stage betatron collimation system [1] consists of the primary collimator (thin foil) which scatters halo particles and the secondary collimators (bulky blocks) which absorb the scattered particles. Taking into account technical aspects of SIS 100 synchrotron [2], the following design of the collimation system has been developed: Collimators have a rectangular aperture with movable jaws The primary collimator is a 1 mm thick tungsten foil The secondary collimators are 40 cm long blocks Simulation of collimation efficiency Conclusion Collimation efficiency = Losses in collimators Losses in lattice 1. secondary collimator 2. Secondary collimator Primary collimator Quadrupole module 18 m The concept of two-stage collimation is considered for protons and fully-stripped ions. dE dx = 4ρZ 2 e 4 m e v 2 n e L LS (ii) The stopping power in a material is calculated using Bethe-Bloch formula. For calculations of the stopping power of high relativistic heavy fully-stripped ions ATIMA code use Lindhard and Soerensen theory [4], which imply several corrections to standard formula L LS : -40 -30 -20 -10 0 10 20 30 40 x [mm] -6 -4 -2 0 2 4 6 x’ [mrad] Primary -40 -30 -20 -10 0 10 20 30 40 x [mm] -6 -4 -2 0 2 4 6 x’ [mrad] 1. secondary -40 -30 -20 -10 0 10 20 30 40 x [mm] -6 -4 -2 0 2 4 6 x’ [mrad] 2. secondary Effect of lattice errors The impact parameter δ is the typical transverse offset from the edge of a primary collimator jaw for the particles impacting the collimator. Impact parameter is proportional to the rate of the emittance growth. The slope of the beam envelope at the location of the primary collimator gives different effective thickness of the foil for different impact parameter. It has been shown that conventional method of betatron halo collimation can be applied for fully-stripped light and heavy ions in the SIS 100 synchrotron. The main reason of higher level of ions leakage with the growing mass number is the increasing momentum losses. After certain level of momentum losses a halo particle in an accelerator could not make one turn to be scattered by the primary collimator again. Impact parameter (i) Angular distribution of the ions scattered in the primary collimator is approximated as Gaussian with the r.m.s. width calculated using the Moliere theory of multiple Coulomb scattering by ATIMA code [3]. (iii) Tracking of halo particles in MAD-X [5] with given accelerator optics and physical aperture. References 0 100 200 300 400 500 600 700 800 900 1000 s [m] 10 -3 10 -2 10 -1 10 0 10 1 10 2 Beam losses [%] 1.SC 2.SC K eff =94.44% 40 Ar 18+ 0 100 200 300 400 500 600 700 800 900 1000 s [m] 10 -3 10 -2 10 -1 10 0 10 1 10 2 Beam losses [%] 1.SC 2.SC K eff =90.189% 40 Ar 18+ 3 4 5 6 7 8 9 10 11 Closed orbit distortion [ mm] 80 85 90 95 100 Collimation efficiency [ %] 12 C 6+ 40 Ar 18+ 84 Kr 36+ 132 Xe 54+ High energy density: 1 GJ/mm 2 Heat impact Heavy ions operation Machine activation Ultra-high vacuum: 10 -12 mbar Vacuum desorption Halo collimation system localizes beam losses and makes machine hands-on maintainable. The primary collimator were transversely placed at 4.5σ r.m.s. of the beam size. Retraction distance (normalized difference of normalized collimators acceptance) has been chosen 0.1 based of previous investigations. Beam losses outside the collimation system in SIS 100 are mainly located in cryo- collimators. The amount of particles taking part in an inelastic nuclear scattering is at the level of 2-4% for light ions and at the level of 4-6% for heavy ions. To estimate the influence of the lattice errors on the collimation performance the closed orbit distortion was included in the particle tracking simulations. Closed orbit distortion with r.m.s. value of 6.8 is a result of transverse positional error of magnets edges. It was found out that after one turn less than 0.1% of ions, which was scattered with the small impact parameter, hit the primary collimator jaw with the same or smaller impact parameter for all ion species. The collimation efficiency of light ions (up to 20 Ne) has almost no dependence on impact parameter. Heavy ions collimation efficiency grows with the increasing impact parameter due to wider angular straggling. After certain value of initial impact parameter collimation efficiency decreases due to growing energy losses. A series of simulations for initial impact parameters in the range of 10 -3 – 3 μm has been performed: Simulation has been performed for 100 different seeds of errors. Closed orbit distortion affects the collimation efficiency of light ions: standard deviation is 5% Heavy ions beams collimation is weakly dependent on closed orbit distortion. Some particles may escape collimators after single pass and be lost in the lattice or be scattered again in the collimation system. Simulations has been performed for beams at the injection energy. Over 99% of light ion (up to 20 Ne) beam losses are located in the collimators. Heavy ions with bigger momentum losses in a primary collimator are lost during one turn in an accelerator. x = 1 mm δ =3μm δ =0.1μm

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Page 1: Ion Beam Collimation for the FAIR Synchrotron SIS100 · 2019. 2. 28. · Beam ) Beam pipe Primary collimator 1. secondary collimator 2. secondary collimator Beam pipe Beam Halo 103

10�3 10�2 10�1 100

Impact parameter [µm]10�1

100

101

102

Frac

tion

ofpa

rticl

eshi

tPC

[%]

12C18+

40Ar18+

84Kr36+

132Xe54+

10�3 10�2 10�1 100

Impact parameter [µm]70

75

80

85

90

95

100

Col

limat

ion

effic

ienc

y[%

]

12C18+

40Ar18+

84Kr36+

132Xe54+

Beam )

Beam pipe

Primarycollimator

1. secondarycollimator

2. secondarycollimator

Beam pipe

Beam

Halo

10�3 10�2 10�1 100

Impact parameter � [µm]10�7

10�6

10�5

10�4

10�3

10�2

10�1

100

��p

/p

1H1+

2H1+

4He2+

12C6+

14N 7+

16O8+

20Ne10+

40Ar18+

84Kr36+

132Xe54+

181Ta73+

197Au79+

1 H 2 H4 H

e12C

14N

16O

20N

e40A

r84K

r13

2 Xe

181 T

a19

7 Au

50

60

70

80

90

100

Col

limat

ion

effic

ienc

y[%

]

multi pass efficiencysingle pass efficiency

10�3 10�2 10�1 100

Impact parameter � [µm]10�2

10�1

100

101

✓ x,r

.m.s

.[m

rad]

1H1+

2H1+

4He2+

12C6+

14N 7+

16O8+

20Ne10+

40Ar18+

84Kr36+

132Xe54+

181Ta73+

197Au79+

0 5 10 15s [m]

-75

-50

-25

0

25

50

75

x[m

m]

PC 1.SC QFQD 2.SC47.7% lost in 1.SC23.7% lost in 2.SC0.0% lost in Quad28.6% escaped

Beam envelope 4.5�

Abstract!

*[email protected] This work is supported by BMBF contract 05P12RDRBM

Ion Beam Collimation for the FAIR Synchrotron SIS100!Ivan Prokhorov*!TEMF, TU Darmstadt, Darmstadt, Germany!!

Ivan Strasik and Oliver Boine-Frankenheim!GSI, Darmstadt, Germany!

The collimation system for the SIS 100 synchrotron has to operate with protons as well as with light and heavy fully-stripped ions (2H1+ - 197Au79+). The concept and basic design features of the betatron halo collimation in SIS 100 were developed previously for proton operation. The main task of the presented work is to compare the efficiency of proton and ion beam collimation. For this purpose multi pass tracking of halo particles was performed using MAD-X including the simulation of scattering process and energy loss in the collimators using the ATIMA code. The collimation efficiency as a function of the ion species together with the detailed beam loss distribution along the ring circumference are presented.!

θr .m.s =13.6MeV

βpcZ x

X 01+ 0.38ln x

X 0( )⎡⎣⎢

⎤⎦⎥

Motivation!Beam halo is non-Gaussian tails of a beam. It occurs due to beam dynamics aspects (beam instabilities, IBS, beam mismatch) and machine imperfections (RF noises, magnet errors and misalignments).!

Principles of collimation!

1.  J.B. Jeanneret, Phys. Rev. ST Accel. Beams 1 (1998) 081001!2.  P. Spiller et al., “Status of the SIS 100 heavy ion synchrotron

project at FAIR”, IPAC’13, Shanghai, May 2013, THPWO011.!3.  http://web-docs.gsi.de/~weick/atima/!4.  A.H. Soerensen J. Lindenhard. Relativistic theory of stopping for

heavy ions. Phys. Rev., A53:2443, 1996. 5.  http://mad.web.cern.ch/!

Collimators in SIS 100!

CERN Accelerator School: Accelerator Physics Advanced Level!Trondheim, Norway!24 August 2013!

The two-stage betatron collimation system [1] consists of the primary collimator (thin foil) which scatters halo particles and the secondary collimators (bulky blocks) which absorb the scattered particles.!

Taking into account technical aspects of SIS 100 synchrotron [2], the following design of the collimation system has been developed: Ø Collimators have a rectangular aperture with movable jaws Ø The primary collimator is a 1 mm thick tungsten foil Ø The secondary collimators are 40 cm long blocks

Simulation of collimation efficiency!

Conclusion!

Collimation efficiency = Losses in collimatorsLosses in lattice

1. secondary collimator

2. Secondary collimator

Primary collimator

Quadrupole module

18 m

The concept of two-stage collimation is considered for protons and fully-stripped ions. !

− dEdx

= 4ρZ2e4

mev 2 neLLS

(ii) The stopping power in a material is calculated using Bethe-Bloch formula. For calculations of the stopping power of high relativistic heavy fully-stripped ions ATIMA code use Lindhard and Soerensen theory [4], which imply several corrections to standard formula LLS:

�40�30�20�10 0 10 20 30 40

x [mm]�6

�4

�2

0

2

4

6

x’[m

rad]

Primary

�40�30�20�10 0 10 20 30 40

x [mm]�6

�4

�2

0

2

4

6

x’[m

rad]

1. secondary

�40�30�20�10 0 10 20 30 40

x [mm]�6

�4

�2

0

2

4

6

x’[m

rad]

2. secondary

Effect of lattice errors!Ø The impact parameter δ is the typical transverse offset from the edge of a primary collimator jaw for the particles impacting the collimator.!Ø Impact parameter is proportional to the rate of the emittance growth.!Ø The slope of the beam envelope at the location of the primary collimator gives different effective thickness of the foil for d i f f e r e n t i m p a c t parameter.!

!

It has been shown that conventional method of betatron halo collimation can be applied for fully-stripped light and heavy ions in the SIS 100 synchrotron. The main reason of higher level of ions leakage with the growing mass number is the increasing momentum losses. After certain level of momentum losses a halo particle in an accelerator could not make one turn to be scattered by the primary collimator again. !

Impact parameter!

(i) Angular distribution of the ions scattered in the primary collimator is approximated as Gaussian with the r.m.s. width calculated using the Moliere theory of multiple Coulomb scattering by ATIMA code [3].!

(iii) Tracking of halo particles in MAD-X [5] with given accelerator optics and physical aperture.

References!

0 100 200 300 400 500 600 700 800 900 1000s [m]

10�3

10�2

10�1

100

101

102

Bea

mlo

sses

[%] 1.SC

2.SC Keff =94.44% 40Ar18+

0 100 200 300 400 500 600 700 800 900 1000s [m]

10�3

10�2

10�1

100

101

102

Bea

mlo

sses

[%] 1.SC

2.SC Keff =90.189% 40Ar18+

3 4 5 6 7 8 9 10 11Closed orbit distortion [mm]

80

85

90

95

100C

ollim

atio

nef

ficie

ncy

[%] 12C6+

40Ar18+

84Kr36+

132Xe54+

High energy density: 1 GJ/mm2 Heat impact

Heavy ions operation Machine activation

Ultra-high vacuum: 10-12 mbar Vacuum desorption

Halo collimation system localizes beam losses and makes machine hands-on maintainable.!

Ø The primary collimator were transversely placed at 4.5σr.m.s. of the beam size. !Ø Retraction distance (normalized difference of normalized collimators acceptance) has been chosen 0.1 based of previous investigations.!

Ø Beam losses outside the collimation system in SIS  100 are main ly l o c a t e d i n c r y o -collimators.!Ø The amount of particles taking part in an inelastic nuclear scattering is at the level of 2-4% for light ions and at the level of 4-6% for heavy ions.!

To estimate the influence of the lattice errors on the collimation performance the closed orbit distortion was included in the particle tracking simulations. Closed orbit distortion with r.m.s. value of 6.8 is a result of transverse positional error of magnets edges.!

Ø It was found out that after one turn less than 0.1% of ions, which was scattered with the small impact parameter, hit the primary collimator jaw with the same or smaller impact parameter for all ion species.!Ø T h e c o l l i m a t i o n efficiency of light ions (up to 20Ne) has almost no dependence on impact parameter. !Ø Heavy ions collimation efficiency grows with the i n c r e a s i n g i m p a c t parameter due to wider angular straggling.!Ø After certain value of initial impact parameter col l imation efficiency d e c r e a s e s d u e t o growing energy losses. !

A series of simulations for initial impact parameters in the range of 10-3 – 3 μm has been performed:!

Ø Simulation has been p e r f o r m e d f o r 1 0 0 different seeds of errors. !Ø Closed orbit distortion affects the collimation efficiency of light ions: standard deviation is 5% !Ø Heavy ions beams collimation is weakly dependent on closed orbit distortion.!

Some particles may escape collimators after single pass and be lost in the lattice or be scattered again in the collimation system.!

Ø Simulations has been performed for beams at the injection energy.!Ø Over 99% of light ion (up to 20Ne) beam losses are located in the collimators.!Ø Heavy ions with bigger momentum losses in a primary collimator are lost during one turn in an accelerator.!

x = 1 mm

� = 3µm

� = 0.1µm