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Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec....

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Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Muon collider meeting, Miami Dec. 13, 2004 Dec. 13, 2004 Slide 1 Slide 1
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Page 1: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Helical Cooling Channel Simulation with ICOOL and G4BL

K. Yonehara

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 1Slide 1

Page 2: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Contents

• Introduction• Simulation results

– ICOOL and G4BL

• Present interesting– Beam dynamics– Low momentum problem– Design RF cavity

• Summary/Next to do

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 2Slide 2

Page 3: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Introduction

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 3Slide 3

Analytical six-dimensional cooling demonstration in the helical cooling channel (HCC) with the high pressure gaseous hydrogen absorber has been done (MuCoolNote0284).

We need to verify the new idea by a numerical method.

ICOOL and G4BL

Page 4: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Introduction

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 4Slide 4

Now we can analyze the beam dynamics in the simulationsand develop the channel for applying to a muon collider.

Page 5: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Collaborators

D. M. KaplanIllinois Institute of Technology, Chicago, IL

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 5Slide 5

M. Alsharo’a, R. P. Johnson, P. Hanlet, K. Paul, T. J. RobertsMuons, Inc., Batavia, IL

K. Beard, A. Bogacz, Y. S. DerbenevJLab, Newport News, VA

Page 6: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

ICOOL and G4BLSpecifications

• ICOOL– Fortran

– Based on Geant3

– Tested many times by many people

– Easy to learn

• G4BL– C++

– Based on Geant4

– Flexible

– Easy to develop

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 6Slide 6

Page 7: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

ICOOL and G4BLHelix coil

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 7Slide 7

Spin rotator coil

Page 8: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

ICOOL and G4BLHelical orbit

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 8Slide 8

Page 9: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

G4BL

ICOOL and G4BLLayout of HCC

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 9Slide 9

Reference orbit

Particle orbit

xy

ICOOL

HCCLength: 10 mPeriod: 1 mRadius: 0.65 m

z

Page 10: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

ICOOL and G4BLSimulation parameters

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 10Slide 10

Parameters Value in simulation for + Unit

Beam momentum, p 200 MeV/c

Solenoid field -5.45 T

Helix period 1.00 m

Helical magnet inner radius 0.65 m

Transverse field at beam center 1.241.24 T

Helix quadrupole gradient -0.206-0.206 T/m

Helix orbit radius, a 0.159 m

Dispersion factor, D 1.7061.706

Accelerating RF field amplitude 33.0 (32.7 in G4BL) MV/m

Frequency 0.201 GHz

Absorber gas pressure 400 atm

Absorber energy loss rate 14.9 MeV/m

Page 11: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 11Slide 11

•These plots include all particles.

ICOOL and G4BLFirst result

Page 12: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 12Slide 12

ICOOL and G4BLSummary

• We first observed the cooling effect of HCC in the simulations which is predicted by the analytical method.

• The simulation result in ICOOL shows a good agreement (discrepancy <10 %) with G4BL.

• This could be a proof test for both codes.

Page 13: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Beam dynamicsNo absorber

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 13Slide 13

dr vs pr z vs drReference orbit

Start point

Page 14: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Beam dynamicsWith GH2 absorber

z vs pr z vs dr

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 14Slide 14z, dt vs dE

Particle direction

Page 15: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Beam dynamicsSummary

• We just start considering this study. We will see more analysis results soon.

• We observe a strong coupling between transverse and longitudinal motions.

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 15Slide 15

Page 16: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Low momentum problemIntroduction

The design of helical cooling channel for a lower momentum muon is practical since it can significantly reduce the strength of helix and solenoid fields. However, we never succeed to see a nice cooling result in a lower momentum region. We noticed that the dispersion factor should be modified to take into account the correction of the energy loss process. This correction should be larger for a lower momentum particle since the energy loss rate of it is larger than that of a higher momentum particle.

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 16Slide 16

Page 17: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Low momentum problemEffective dispersion factor

Deff = Dlattice + Deloss

Dlattice =

Deloss =

ap

dp

da

dE/ds

pdp

d(dE/ds)

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 17Slide 17

Page 18: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

p

(MeV/c)

150 -0.483

200 -0.265

250 -0.138

374 0.0

Deloss

Low momentum problemEstimate Deloss

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 18Slide 18

Page 19: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Low momentum problemAnalysis of simulation results

Use quadratic functionfor curve fitting:Easy to extract the peakposition

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 19Slide 19

Merit factor= cooling facter Transmission efficiency

+

Page 20: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Low momentum problemAnalyzed result

p (MeV/c)Peak position

(fitting curve)

Distance

from 374 MeV/c

Dispersion factor by energy loss

Fraction between columns 4 & 5

374 0.229 0.0 0.0

250 0.0697 -0.160 -0.138 0.86

200 -0.0962 -0.326 -0.265 0.81

150 -0.321 -0.550 -0.483 0.88

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 20Slide 20

Page 21: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Low momentum problemSummary (1)

• The additional dispersion factor caused by the energy loss effect well reproduces the peak position in the merit factor curve.

• However, we still see a small fraction in the effective dispersion factor. This could be caused by another dispersion effect.

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 21Slide 21

Page 22: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Low momentum problemEvolution of emittances

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 22Slide 22

Page 23: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Low momentum problemAcceptance and Equilibrium emittance

p (MeV/c)

Initial/Final

tran (mm rad)

Initial/Final

long (mm)

Initial/Final

6D (mm3)p/p

374 27.8/3.36 71.0/7.68 48900/57.4 120/374

250 22.5/1.96 73.9/2.72 32000/6.62 60/250

200 18.3/1.91 66.4/2.47 17500/5.15 55/200

150 14.3/2.98 48.3/5.86 8660/20.0 45/150

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 23Slide 23

Page 24: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Low momentum problemSummary (2)

• The acceptance of higher momentum beam is larger but the cooling decrement is smaller while the cooling decrement in lower momentum beam is larger but the acceptance is smaller.

• So the optimum beam momentum seems to be 200 ~ 250 MeV/c.

• The optimum beam momentum can be changed by the absorber density (pressure).

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 24Slide 24

Page 25: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Design RF cavity

• Install bessel function type RF cavities in the simulation– Frequency

> 200, 400, 800, and 1600 MHz.– Location

> We tested two types of location of the center of RF cavities; one is on an HCC axis (no offset) and the other is on a reference orbit (with offset).

– Shape> We design a unique shape of RF cavities. We will

discuss them in future. Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 25Slide 25

Page 26: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Design RF cavityOffset RF

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 26Slide 26

No offset

With offset

+

+

12

3 4 5

1

2

3

45

Page 27: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 27Slide 27

Design RF cavityEvolution of emittance

frequency = 0.2 GHzCavity radius ~ 0.6 m

Page 28: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Design RF cavitySimulation result

p (MeV/c)Initial/Final

tran (mm rad)

Initial/Final

long (mm)

Initial/Final

6D (mm3)

Uniform Ez 18.3/1.88 64.0/2.42 17200/4.83

With offset 18.9/1.57 74.1/4.54 20100/6.46

No offset 16.2/5.46 64.0/3.85 12800/41.1

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 28Slide 28

Page 29: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

• The RF cavities with offset works well.

• However, we observe a less reduction of the longitudinal emittance by using the offset type RF cavities.

• We need to improve the propagation of longitudinal beam cooling in HCC.

Design RF cavitySummary

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 29Slide 29

Page 30: Helical Cooling Channel Simulation with ICOOL and G4BL K. Yonehara Muon collider meeting, Miami Dec. 13, 2004 Slide 1.

Summary/Next to do

• The two simulations work pretty well. • We study beam dynamics in HCC. • We found the effective dispersion factor. • We design several type of RF cavities. • We figure out the matching problem.

Muon collider meeting, MiamiMuon collider meeting, MiamiDec. 13, 2004Dec. 13, 2004 Slide 30Slide 30


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