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The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

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Page 1: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

The Emittance Growth Scaling Laws in Resonance Crossing

X. Pang, F. Wang, X. Wang, S.Y. LeeIUCF, Indiana University

K.Y. NgFermilab

1

Page 2: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Introduction FFAG → a favorable candidate for high power proton driver.

Constant guide field → rep rate can be very high, in the kHzs.

Scaling design nonlinear fields, large magnet apertures.

→ fixed tune, but fringing field or flux saturation in iron

poles can cause tune change.

Non-scaling design linear fields, much smaller magnet apertures.

tunes change by many units in a ramp cycle.

Beam quality can deteriorate when crossing resonances.

Tune-ramp rate

typically ~ -10-4 to -5*10-3 per turnn

E

Enzxzx

2

,,

2

Page 3: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Example Ruggiero suggested 3 concentric FFAGs as a proton driver to replace BNL AGS to reach

10 MW beam power.

Tunes change from

(νx, νz) = (40,38.1) to (19.1,9.3)

Cross systematic 4th and 6th

resonances: (P=136)

4νx=P, 4νz=P, 2νx+2νz=P

6νx=P, 6νz=P, 2νx+4νz=P, 4νx+2νz=P

S.Y. Lee pointed out emittance

growth can be large if crossing

rate is slow, and gave a scaling relationship.

Thus phase advance per cell cannot be near 900 and 600.

Lattice design can become very restricted.3

Page 4: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

The Model Lee, et al. studied sp-ch driven 4th order systematic resonances and field-error

driven linear resonances.

We study here sp-ch driven 6th order systematic resonances and octupole driven

4th order parametric resonances.

Our study bases on simulations.

Lattice is similar to Fermilab Booster, with P = 24 FODO cells.

Sp-ch kicks applied at the center of D and F quadrupoles, two kicks per

superperiod. (Making 4 kicks per superperiod does not change our results)

Transport matrices used from magnet to magnet.

Kinetic energy fixed at 1 GeV, tunes allowed to ramp.

Syn. oscillation neglected since emittance usually grows much faster.

Assume bi-Gaussian distribution:

4

Page 5: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Systematic Resonances Sp Ch potential:

Taylor’s Expansion:

Each particle passing through a length ∆s experiences a space-charge kick:

4th order

6th order

5

Page 6: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Space Charge Force

In our simulation:• not round beam complex error function• round beam power series

If the beam is not round beam, it is straightforward to show

. ,2

2 ,

)(2 ,

)(2

],2

1[)( Where

)],()([)(

2

,2

zx

2

22

2222

0

)()(

22

''

22

22

x

z

x

z

zxzx

ZZ

r

bjarjba

zx

sc

scsc

rt

tv

zb

xa

dej

eZw

r

bjarwejbawjF

FK

sj

s

singularity when r=1

6

Page 7: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Space Charge Force For round beam, we need to expand the space-charge force around sx=sz

or r=1.

t

tv

zb

xa

ev

dv

r

rzxf

edvr

zxf

zxfz

Kz

VF

zxfx

Kx

VF

x

z

zxzx

vbva

rz

vbva

rx

z

z

scsc

scz

x

x

scsc

scx

2

22

2222

)11

()1(1

22

222

)11

()1(1

222

222,

222,

2

2 ,

)(2 ,

)(2 where

1

),(

1

1),(

),(

),(

2222

2222

x

zxr

1

/)1( , ]

)1)((

)2/1(

)(

)2/1(exp[ ),(

1

0 2

2222 vt

t

ttzttxdtzxf

zxxzxxzx

xx

7

Page 8: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Space Charge Force• Do Taylor’s Expansion and using the integral:

We obtain:

)( ,

)( ,, )2

!1(

!)(

221

00

1zxxzxx

n

k

kw

nnwt

n

zq

xpqpw

k

we

w

ndttewf

)}.()](3840

)3()(

24

)3(

)](16

93465)(

2

193)(

2

7[

)](384

)3()(

4

)3()(

4

235)(3[

)](48

)3()()3()(

2

5[

)](8

)3()(2[)(

2

3)({),(

610

5

9

3

8

322

7

2

65

8

4

7

2

6

2

54

6

3

543

4

2

32

2022

Owfqp

wfqqp

wfqpqqp

wfqpq

wqf

wfqp

wfqqp

wfqpq

wqf

wfqp

wqfqpwfq

wfqp

wqfwfqp

wfzxfzx

xx

ysingularit theremove to

!)1(

)()(

use small, is Whenever

0. beam theofcenter

at the resides particleWhen

0

k

k

n kkn

wwf

w

w

An expansion up to O(e3) together with e ≤0.01 will provide a space chargeforce that is accurate up to one part in one million.

8

Page 9: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Space Charge Force• To ensure the accuracy of our calculation of the space charge force, we

compare the computed space charge force using complex error function and series with results obtained by direct numerical integration.

Integrals converge

To cope with the infinite upper limits,transform the variable to u=1/(t+1)

sx=1cm, sz=0.5cm sx=1cm, sz=0.99cm

Numerical integrations are still too time-consuming for systematic paramatric studies.

9

Page 10: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

In action-angle variables,

Can factor out sp-ch dependent part of resonance strength, giving dimensionless reduced strength gmnl:

sp-ch dependentlattice dependent

6nx= P

6nz= P

6th order Systematic Resonance

10

Page 11: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Simulation Parameters

• Proton injection rate particles per turn.• Harmonic number h= 84.• Circumference C=474.2m.• Bunching factor • Initial emittance: • Kinetic energy is kept constant at 1GeV during

the tracking.

11104

2)2/( shCB

mrmsN 6, 1033.8

11

Page 12: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

100 turns injection Crossing systematic

resonances:

6nx=P, 6nz=P, P=24

dnx,z/dn = -0.0004

Aperture=

Emittance growth factor

(EGF):

Final emit./initial emit.

Sample Simulation

)(3.69,3.89)ν,(ν

)(4.25,4.45)ν,(ν

zx

z0x0

Turn 820

Turn 127000172.0||

00181.0||

06

60

P

P

g

g

mradmm 500

12

Page 13: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Scaling Power Laws Tune ramp rate:0.0004 0.0112

Log-log plots

Scaling Law

Critical tune ramp rate

13

Page 14: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Critical Tune Ramp Rate

Can serve as a guideline for FFAG design!

At the critical tune ramp rate, emittance is almost unchanged.

Emittance ~ G∙∆n constantG : resonance strength∆n: number of turn under the influence of resonance.

G~ g∙∆nsc

∆n ~ ∆nsc /|dn/dn|c

14

Page 15: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Similar scaling law for the 4th order Systematic Resonances

15

Page 16: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Conclusion

Power scaling laws obtained between EGF and dnz/dn for

crossing sp-ch driven systematic 6th order resonances

For a ring like Fermilab Booster,

with |g60P|~0.00118, Dnsc,x=0.30, |dnx/dn|crit~0.006/turn

with kinetic energy 1GeV, and nx =4, (dE/dn)crit ~ 2.2MeV

Solution:

Design a machine with smaller stopband!

16

Page 17: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

What if we have more space-charge kicks

The effect of the space chargekicks should essentially dependon the harmonic content.

17

Page 18: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

4th Order Parametric Resonance One octupole is added at D-magnet in last cell to mimic random 4th order parametric

resonance. Potential: In action-angle variables:

Octupole kick:

Dimensionless reduced resonant strength:

4nx= l

4nz= l

18

Page 19: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Simulation Parameters

• Kinetic energy 1GeV• Octupole strength S4 = 50 m-3, pole tip field

0.035T with aperture 5cm and length 1m.• Placed at defocusing Quadrupole.• 3 × 1011 particles are injected per turn.• Tracking for 1200 turns. Initial tune (vx0,vz0)=(6.975,6.875)

19

Page 20: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Sample Simulation bx,D=6.3m, bz,D=21.4m S4=20m-3

70 –turn injection

The space charge turn shift: (∆vsc,x , ∆vsc,z )=(0.167,0.165)

Bare tunes are ramped down from 100th turn at a rate of:

Heavy beam loss is observed 6.5% during 1200 turns

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Page 21: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Scaling Power Laws

Critical tune ramp rate

21

Page 22: The Emittance Growth Scaling Laws in Resonance Crossing X. Pang, F. Wang, X. Wang, S.Y. Lee IUCF, Indiana University K.Y. Ng Fermilab 1

Critical Tune Ramp Rate Octupole driven 4th order resonance: 4vz = 27

Given Dnsc,z and |g04l|,

this gives min. tune ramp

rate so that EGF remains

tolerable.

It is clear that sp-ch

contribution is significant.

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