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Yujong Kim The Center for High Energy Physics, Korea DESY Hamburg, Germany [email protected], http://www.desy.de/~yjkim Alternative Bunch Compressors for ILC TESLA-S2E-2005-65 July 12 th , 2005, The 8 th ACFA Workshop, Daegu, Korea
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Yujong Kim The Center for High Energy Physics, Korea DESY Hamburg, Germany

Jan 16, 2016

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July 12 th , 2005, The 8 th ACFA Workshop, Daegu, Korea. Alternative Bunch Compressors for ILC. Yujong Kim The Center for High Energy Physics, Korea DESY Hamburg, Germany. [email protected], http://www.desy.de/~yjkim. TESLA-S2E-2005-65. - PowerPoint PPT Presentation
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Page 1: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

Yujong Kim

The Center for High Energy Physics, Korea

DESY Hamburg, Germany

[email protected], http://www.desy.de/~yjkim

Alternative Bunch Compressors for ILC

TESLA-S2E-2005-65

July 12th, 2005, The 8th ACFA Workshop, Daegu, Korea

Page 2: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

2

Contents

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Why we need Bunch Compressor (BC) for the ILC project ?

Working Principle of Bunch Compressor

Several Important Considerations to design Bunch Compressor for the ILC

Incoherent Synchrotron Radiation (ISR) Coherent Synchrotron Radiation (CSR) Nonlinearities (RF curvature, short-range wakefields, T566, space charge effect) RF Jitter Sensitivity and Tolerance

Current Bunch Compressor in TESLA TDR

Alternative Bunch Compressors for the ILC Project

1st Alternative BC (13NOV04 Version) to compress σz,i= 6.0 mm to 300 µm 2nd Alternative BC (04APR05 Version) to compress σz,i= 9.0 mm to ~ 100 µm 3rd Alternative BC (09JUL05 Version) to compress σz,i= 6.0 mm to 150 µm

Summary and Acknowledgements

Page 3: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

3

emittanceverticalnormalized

ungbeamstrahltoduelossenergyrelative

powerbeamaverage

energymassofcenter

2~factortenhancemenpinch

(IP)pointninteractioatsizebeam

frequencyrepetitionpulse

bunchperparticlesofnumber

pulseperbunchesofnumber

m1074.54

*yx,

*

2/1

,

3/2-20**

2

n,y

BS

repbbcmb

cm

D

rep

b

b

zyDyn

BS

cm

bD

yx

repbb

fNnEP

E

H

f

N

n

forHE

PH

fNnL

For given center of mass energy Ecm and fractional beamstrahlung loss δBS

- higher average beam power Pb

- smaller vertical emittance εn,y

- smaller vertical beam size at IP σ*y

- shorter bunch length σz = smaller β*n,y (hourglass effect, )

give higher higher luminosity L.

According to Tor Raubenheimer’s new suggested ILC beam parameters range, we should compress bunch length from 6.0 mm to 0.15 mm for high luminosity mode operation (compression factor = 40).Recently, Andy Wolski suggested to use 9.0 mm length in damping ring. In this case, compression factor from 9.0 mm to 0.15 mm is 60.

zy *

Why we need BC in ILC Project ?

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Luminosity L (TESLA TDR 2001):

To supply e+e- colliding beams with high luminosity of a few 1038 m-2s-1

Page 4: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

4

Working Prinicple of Bunch Compressor (BC)

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Bunch Compressor Layout for SCSS Project - Y. Kim et al, NIMA 528 (2004) 421

chicane. bendr rectangulathefor2

3where

))/(()/()/(

56566

3256656

RT

EdEEdETEdERdzdz iiiif

)3

2(2 2

56 BB LLR

dt

dETail

Head

from precompressor linac from chicane

Page 5: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

5

Incoherent Synchrotron Radiation (ISR) is generated when relativistic long beam goes through dipole magnet. Since ISR is a random quantum process, it generates incoherent (= slice, or uncorrelated) energy spread, hence slice emittance growth in the bending plane. For one dipole magnet, the relative uncorrelated energy spread due to ISR is given by

Slice emittance growth due to ISR is given by

Considerations - ISR in Dipole

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

.)GeVm1013.4(1 355-211

dipole1,, BB

ISR EL

Electron pathDipole region

chicane.for3

)(108 minmax2

568

BB

Bx LL

LE

- lower energy- longer dipole- smaller bending angle are good against ISR effects

bISR NP

Page 6: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

6

Considerations - CSR in BC

In BC where dispersion is nonzero, bunch length becomes smaller.Short electron bunches in dipole can radiate coherently (CSR) at wavelength CSR from tail electrons can overtakes head electrons after the overtaking length.

CSR generates correlated energy spread along whole bunch:

Electrons are transversely kicked at the nonzero dispersion region or in BCHence, projected emittance is increased in BC due to CSR.

.radiusbendingis,lengthbunchrmsiswhere 243/12

OT RRL zz

3432dipole1 220 /

z/

Be,

R

NLr.

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

z

Electron path

CSR from tailTail

LOT Head

E

dEx

x

xx

BCin0

Dipole region

2bCSR NP

Page 7: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

7

Considerations - CSR in BC

Without CSR self-interaction

With CSR self-interaction

DM3 DM4DM2DM1

Head : energy gain by CSR

Tail : energy loss due to CSR

Head with lower energy

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

x

z

Projected emittance growth due to CSR

E

dEx

x

xx

BCin0

Courtesy of M. Dohlus

Page 8: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

9

Considerations - Nonlinearities

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Blue : After BC for different compressionGreen : Before BC

Without higher harmonic compensation cavity, nonlinearity in dz-dE chirping becomes stronger after BC, and there is some local charge concentration in very small local region. This nonlinearity by RF curvature makes femtosecond spike at TTF2.

))/(()/()/( 3256656 iiiif EdEEdETEdERdzdz

Page 9: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

10

Considerations – Nonlinearities

Linearization of longitudinal phase space with a higher harmonic cavity

number.harmonic the is and linac,frequencylowthe of gain

energy is cavity,harmonichighertheofgainenergytheiswhere

cos)/(0)(

)(

)(

12

12

12

02

21

22

n

GLGL

nGLGLdzd

dEdEd

dzd

ds

dz

Linear range ~ 60 degree 60 deg in 2856 MHz ~ 60 ps (18 mm)60 deg in 1300 MHz ~ 126 ps (37.8 mm)60 deg in 650 MHz ~ 252 ps (75.6 mm)Good for 9.0 mm (rms) ILC bunch

C-band Linac + X-band Correction Cavity

Only C-band Linac

“-” means deceleration !

-70 MeV deceleration

SCSS BC

Y. Kim et al, NIMA 528 (2004) 421

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Nonlinearities in the longitudinal phase space due to RF curvature, short-range wakefields, T566, and space charge force can be compensated by harmonic cavity.

Page 10: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

14

BCs for European XFEL (13JAN04 Version)

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

ACC1 ACC2 ACC4 ACC5RF-GUN

Q=1.0 nC e-beam

0.0 m 12.0444 m

ASTRA with Space Charge

11.5 MV/m25.0 MV/m-18.3 deg

34.8 MV/m160.6 deg

ACC39

60 MV/m38 deg

ACC6ACC3BC1

z = 1.76 mm 113 m 23 m

E = 510 MeV ~ 1.89%R56 = 87 mm = 3.95 deg

E = 510 MeV ~ 1.88%R56 = 4.8 mm = 0.93 deg

ACC7 ACC8 ACC118

UNDULATOR, 200 mz = 20.5 m

1567 m

20.65 MV/m0.0 deg

All projected parameters !E = 20.0 GeV = 0.008%x= 37.3 m, y= 31.6 m, z = 20.5 m nx= 1.15 m, ny= 0.94 m

BC2

ACC9

20.5 MV/m-29.6 deg

20.65 MV/m0.0 deg

To the end of Linac : ELEGANT with CSR with geometric wakefields

without space charge

FODO MODULES (90 deg)

With TESLA XFEL Injector, n= 0.9 m

Page 11: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

15

Considerations – RF Jitter Tolerance

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

ACC234 Phase is the most sensitive jitter source to saturation powerand saturation length

For ± 0.5 deg change in ACC2 phase

strong over-compression against ACC234 phase errorLayout with two BC stages is more safer against RF jitter

European XFEL (13JAN04 Version) with a double chicane

Page 12: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

17

New BCs for XFEL (10AUG04 Version)

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

ACC1 ACC2 ACC4RF-GUN

Q=1.0 nC e-beam

0.0 m 12.9869 m

ASTRA with Space Charge

12.8 MV/m24.84 MV/m

-25.0 deg

34.5 MV/m165.9 deg

ACC39

60 MV/m40.0 deg

ACC5 ACC6ACC3BC1

E = 518 MeV ~ 1.87%R56 = 87 mm = 3.95 deg

E = 518-760-1100 MeV ~ 1.87-1.33-0.9%R56 ~ 5.3 mm ~ 0.93 deg

ACC7 ACC8 ACC120

UNDULATOR, 250.1 mz = 21.6 m

1579 m

20.38 MV/m0.0 deg

All are projected parameters !

E = 20.0 GeV = 0.0088%x= 34.2 m, y= 29.5 m, z = 21.6 m nx= 1.044 m, ny= 0.896 m

BC2

ACC9

z = 1.72 mm 94 m 21.6 m

20.2 MV/m-25.0 deg

0-20.5-35 MV/m-44.5 deg

To the end of Linac : ELEGANT with CSR with geometric wakefields

without space charge

FODO MODULES (90 deg)

With New European XFEL Injector, n= 0.88 m

Page 13: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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Considerations – Jitter under Random Errors

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

400 Times Tracking with (13JAN04) 400 Times Tracking with (10AUG04)

wider change in bunch length for (13JAN04 Version)stronger correlation with errors in other components !

most sensitive jitter source on bunch length = ACC2 phase error

Page 14: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

20

Considerations – Jitter under Random Errors

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

400 Times Tracking with (13JAN04) 400 Times Tracking with (10AUG04)

wider change in bunch arriving time for (13JAN04 Version)stronger correlation with errors in other components !

most sensitive jitter source on arriving time = BC1 current error

Page 15: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

21

Current ILC Bunch Compressor in TDR

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

- One stage : sensitive to RF jitter- Many dipoles : twelve dipoles with 3.23 deg bending angle & six dipoles with 6.46 deg- Large energy spread due to ISR and CSR from many dipole, hence emittance growth- No consideration of short-range wakefields in TESLA modules (under estimation) - No effective nonlinearity compensation- Many dipoles and QMs, which induce chromatic effects

BC ParametersEnergy ~ 5.0 GeVCharge = 3.2 nCInitial energy spread at DR exit = 0.13%Initial rms bunch length = 6 mmFinal rms bunch length = 0.3 mmMomentum compaction R56 = 215 mmCompression factor = 20Initial horizontal emittance = 8.0 µmInitial vertical emittance = 0.02 µm

Periodically dispersion : emittance compensation

Page 16: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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1st Alternative BC for ILC (10NOV04 Version)

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Final parameters

E = 6.0 GeV = 2.173%z = 300 m nx= 8.7 m, ny= 0.02 m

z = 6.00 mm 673 m 300 m

ACC1 ACC2 ACC4

Q=3.2 nC e-beam

23.4 MV/m-45 deg

24.8 MV/m170.0 deg

ACC5 ACC6ACC3BC1

E = 5.689 GeV ~ 2.4%R56 = 236 mm = 5.3 deg

E = 6.0 GeV ~ 2.174%R56 ~ 17 mm ~ 1.4 deg

BC2

13.3 MV/m-21.5 deg

Up to main linac : ELEGANT with CSR, ISR, and geometric short-range wakefields.but without space charge

Initial parameters

E = 5.0 GeV = 0.13% (small !)z = 6.0 mm nx= 8.0 m, ny= 0.02 m

1/8.9 1/2.2

Damping Ring

ACC39

Page 17: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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1st Alternative ILC BC – Chicane Layout

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

From various experiences in Start-To-End simulations and BC designs for TTF2, European XFEL, SCSS, PAL XFEL, we have chosen two BC stages

BC2 has same layout

Page 18: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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1st Alternative ILC BC – Long. Phase Space

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

HeadTail

10NOV04 Version

strong nonlinearity due to RF curvature

Page 19: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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1st Alternative ILC BC – Long. Phase Space

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

HeadTail

10NOV04 Version

Linearization with two ACC39 modules (3.9 GHz) is not enough !

bunch length

z = 6.00 mm z = 673 m

Page 20: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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1st Alternative ILC BC – Long. phase space

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Edges : over (or under)-compression by the nonlinearity due to wakefields, T566, RF curvature

10NOV04 Version

z = 673 µm z = 300 m

Page 21: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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1st Alternative ILC BC – Compression Ratio

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

8.9 times compression at BC1

2.2 times compression at BC2

10NOV04 Version

= 2.173%

Page 22: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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1st Alternative ILC BC – Projected Emittance

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

final horizsontal emittance = 8.7 µm

final vertical emittance = 0.02 µm

10NOV04 Version

even rms horizontal emittance is increased to 8.7 µm due to ISR and CSR but vertical emittance is almost const (0.02 µm).

with consideration of CSR and ISR

Page 23: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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1st Alternative ILC BC – Zoomed after BC2

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Edges : over (or under) -compression due to the nonlinearity

10NOV04 Version

It seems that 3rd harmonic cavity is not enough to compensate the nonlinearity

Page 24: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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Nonlinearity Compensation with 3rd Harmonic

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

~ 60 deg in fundamental RF frequency

60 deg (FW) in 1300 MHz Linac- corresponding to 126 ps (FW)- corresponding to 37.8 mm (FW)- corresponding to 6.3 mm (RMS) (close to current σz = 6.0 mm)

60 deg (FW) in 650 MHz Linac- corresponding to 252 ps (FW)- corresponding to 75.6 mm (FW)- corresponding to 12.6 mm (RMS) (wider than σz = 9.0 mm)- corresponding 3rd harmonic = 1950 MHz

Here Full Width (FW) ~ six times of RMS

Linear range of current compensation layout (1300 MHz + 3900 MHz) is very close to the initial bunch length of 6.0 mm (RMS). With this layout, we can not compensate the nonlinearity well if the initial bunch length is 9.0 mm (RMS).

Page 25: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

31

Nonlinearity Compensation with 2nd Harmonic

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Linear range of a new compensation layout (650 MHz + 1300 MHz) is a wide range of 85 deg. With this layout, we can compensate the nonlinearity properly even though the initial bunch length is 9.0 mm (RMS).

~ 85 deg in fundamental RF frequency

85 deg (FW) in 1300 MHz Linac- corresponding to 178.5 ps (FW)- corresponding to 53.55 mm (FW)- corresponding to 8.93 mm (RMS) (not enough for σz = 9.0 mm)

85 deg (FW) in 650 MHz Linac- corresponding to 357 ps (FW)- corresponding to 107.1 mm (FW)- corresponding to 17.9 mm (RMS) (much wider than σz = 9.0 mm)- corresponding 2nd harmonic = 1300 MHz

Here Full Width (FW) ~ six times of RMS

Page 26: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

32

2nd Alternative ILC BC - (04APR05 Version)

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Frequency of precompressor linac (before BC1) = 650 MHz

Frequency of compensation cavity = 1300 MHz (2nd harmonic of 650 MHz)

Frequency of main linac from down stream of the 2nd bunch compressor = 1300 MHz

Chicane type = S-type to control dispersion within about 1.0 m and to compensate the projected emittance growth due to CSR

Initial bunch length = 9.0 mm (rms)

Final bunch length = 100 µm (rms) with 1.4 deg bending angle at BC2 138 µm (rms) with 1.35 deg bending angle at BC2

1300 MHz TESLA module can replace 650 MHz SACC56

Page 27: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

33

2nd Alternative ILC BC – (04APR05 Version)

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Final parametersE = 6.0 GeV = 2.0491%z = 138 mnx= 9.2 m, ny= 0.02 m

z = 9.00 mm 624 m 138 m

SACC12

Q=3.2 nC e-beam

13.3 MV/m-60 deg

25.1 MV/m160.5 deg

SACC34SBC1

E = 5.370 GeV ~ 2.26%R56 ~ 372 mm = 5.3 deg

E = 6.0 GeV ~ 2.05%R56 ~ 24 mm = 1.35 deg

SBC2

13.3 MV/m-20.0 deg

Up to main Linac with ELEGANT under CSR, ISR, and geometric short-range wakefields. but without space charge

Initial parametersE = 5.0 GeV = 0.13% (small !)z = 9.0 mm nx= 8.0 m, ny= 0.02 m

1/14.4 1/4.5

Damping Ring

ACC1650 MHz 650 MHz 650 MHz

SACC56

Here from SACC12 to SACC56 are two 650 MHz subharmonic modules with 12 cavities, and ACC1 is the 1300 MHz TESLA module with 12 cavities. From the downstream of SBC2, we will use the 1300 MHz TESLA module for the main linac.

ACC2 ACC31300 MHz

Page 28: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

34

2nd Alternative ILC BC – Twiss Parameters

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

dispersion is within ±1.0 memittance growth due to CSR is compensated by reversed dispersion

S-type BC1 chicane = 6 dipoles S-type BC2 chicane = 6 dipoles

Too small modules for FODO cells Too small modules for FODO cells

Page 29: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

35

2nd Alternative ILC BC – Long. Phase Space

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

edge-to-edge ~ 42 mm for 2σ cutting in initial beam distribution

04APR05 Version

reduced nonlinearity due to weaker wakefieldand weaker RF curvature in 650 MHz linac !

Page 30: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

36

2nd Alternative ILC BC – Long. Phase Space

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Nonlinearity was compensated by 1300 MHz TESLA module (ACC1)

z = 9.00 mm z = 624 m

04APR05 Version

Page 31: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

37

2nd Alternative ILC BC – Long. Phase Space

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

z = 624 µm z = 138 m for 1.35 deg at SBC2 z = 100 m for 1.40 deg at SBC2

04APR05 Version

Page 32: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

38

2nd Alternative ILC BC – Energy Spread

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

04APR05 Version

BC1 BC2

z = 9 mm

z = 138 m

= 2.0491%

Page 33: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

39

2nd Alternative ILC BC – Projected Emittance

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

04APR05 Version

final horizontal emittance = 9.2 µm

final vertical emittance = 0.02 µm

BC1 BC2

Page 34: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

40

2nd Alternative ILC BC – CSR & ISR Effects

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

04APR05 Version

horizontal emittance = 8.68 µm 8.04 µm

vertical emittance = 0.02 µm 0.02 µm

BC1 BC2 BC1 BC2

Action of CSR and ISR when we compress σz = 9.0 mm to 138 µm Final horizontal emittance with consideration of CSR and ISR = 9.2 µm Final horizontal emittance with consideration of only ISR = 8.68 µm Final horizontal emittance without consideration of CSR and ISR = 8.04 µm

Page 35: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

41

2nd Alternative ILC BC – Peak Current

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

z = 138 m with 3.2 nCz = 9.0 mm with 3.2 nC

04APR05 Version

good compensation by ACC1good symmetric peak current

Page 36: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

42

3rd Alternative ILC BC - (09JUL05 Version)

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Frequency of precompressor linac = 650 MHz

Frequency of compensation cavity = 1300 MHz (2nd harmonic of 650 MHz)

Frequency of main linac from down stream of the 2nd bunch compressor = 1300 MHz

Chicane type = S-type to control dispersion within about 1.0 m and to compensate the projected emittance growth due to CSR

Initial bunch length = 6.0 mm (rms)

Final bunch length = 150 µm (rms)

Final relative rms energy spread = 1.44% (reduced !)

Page 37: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

43

3rd Alternative ILC BC – (09JUL05 Version)

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

Final parametersE = 6.0 GeV = 1.44%z = 150 m nx= 8.8 m, ny= 0.02 m

z = 6.00 mm 500 m 150 m

SACC12

Q=3.2 nC e-beam

13.3 MV/m-61 deg

25.1 MV/m160.5 deg

SACC34SBC1

E = 5.345 GeV ~ 1.57%R56 ~ 351 mm = 5.15 deg

E = 6.00 GeV ~ 1.44%R56 ~ 24 mm = 1.35 deg

SBC2

13.35 MV/m-26.0 deg

Up to main Linac with ELEGANT under CSR, ISR, and geometric short-range wakefields. but without space charge

Initial parametersE = 5.0 GeV = 0.13% (small !)z = 6.0 mm nx= 8.0 m, ny= 0.02 m

1/12 1/3.3

Damping Ring

ACC1650 MHz 650 MHz 650 MHz

SACC56

Here from SACC12 to SACC56 are two 650 MHz subharmonic modules with 12 cavities, and ACC1 is the 1300 MHz TESLA module with 12 cavities. From the downstream of SBC2, we will use the 1300 MHz TESLA module for the main linac.

ACC2 ACC31300 MHz

Page 38: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

44

3rd Alternative ILC BC – Long. Phase Space

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

z = 6.00 mm z = 150 m

Nonlinearity was compensated by 1300 MHz TESLA module (ACC1)

09JUL05 Version

Page 39: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

45

3rd Alternative ILC BC – Peak Current

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

z = 6.00 mm with 3.2 nC z = 150 m with 3.2 nC

09JUL05 Version

Page 40: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

46

3rd Alternative ILC BC – Energy Spread

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

09JUL05 Version

BC1 BC2

z = 6 mm

z = 150 m

= 1.44%

Page 41: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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3rd Alternative ILC BC – Projected Emittance

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

09JUL05 Version

final horizontal emittance = 8.8 µm

final vertical emittance = 0.02 µm

Page 42: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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Summary

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider

To supply e+e- colliding beams with a high luminosity, we should compress bunch length down to 150 µm by bunch compressors.

To optimize BCs, we should consider various things such as ISR, CSR, nonlinearity, chicane type, compression ratio, energy spread at BCs, Twiss parameters around BCs, and chromatic effect.

We choose 2 BC stages to reduce jitter sensitivity and construction cost. 3 BC stages is expensive and it is not effective if nonlineariy in the longitudinal phase space is not compensated properly.

A shorter linac with a lower frequency BCs will be proper to avoid over-compression at BC2 due to longitudinal short-range wakefields and to reduce construction cost. Linac with a lower frequency also help in reducing jitter sensitivity.

For 2nd and 3rd alternative bunch compressors, we choose subharmonic cavity with 650 MHz as a precompressor linac (before BC1) to compress a bunch with σz = 9.0 mm (rms) to 100 µm or more shorter without any big problem.

Page 43: Yujong Kim The Center for High Energy Physics, Korea  DESY Hamburg, Germany

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The 3rd alternative bunch compressor can compress a bunch with σz = 6.0 mm (rms) to 150 µm or more shorter with a lower final energy spread of 1.44%.

We should consider CSR as well as ISR to estimate realistic BC performance.

To reduce horizontal emittance growth at the ILC bunch compressor more, we will optimize beam energy at BC2, optics around BCs, and chicane type and layout further.

Y. Kim sincerely thanks Professor Dongchul Son, K. Flöttmann, and M. Dohlus for their encouragements of this work and many useful comments and discussions.

Summary & Acknowledgments

TeV-Energy Superconducting Linear Accelerator Projects - TTF-2, TESLA X-ray FEL, TESLA Linear Collider