Space charge studies based on beta measurement in J-PARC MR K. Ohmi - - PowerPoint PPT Presentation

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Space charge studies based on beta measurement in J-PARC MR K. Ohmi - - PowerPoint PPT Presentation

Space charge studies based on beta measurement in J-PARC MR K. Ohmi KEK, Accelerator Lab Dec. 10, 2015, talk at Fermilab K. Ohmi (KEK) Space charge on measured beta Dec. 10, 2015, talk at Fermilab 1 / 36 Overview Hamiltonian and Resonances


slide-1
SLIDE 1

Space charge studies based on beta measurement in J-PARC MR

  • K. Ohmi

KEK, Accelerator Lab

  • Dec. 10, 2015, talk at Fermilab
  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

1 / 36

slide-2
SLIDE 2

Overview

1

Hamiltonian and Resonances Action variable representation Standard model

2

Space Charge force and its Hamiltonian Tune shift and tune slope Resonance terms

3

Lattice nonlinearity Tune shift and tune slppe Resonance terms

4

Superperiodicity Breaking of the superperiodicity Beta function measurement

5

Simulation using the resonance Hamiltonian Without Synchrotron Motion With Synchrotron Motion

6

Summary

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

2 / 36

slide-3
SLIDE 3

Hamiltonian and Resonances

Introduction

Particles move with experience of electro-magnetic field of lattice elements and space charge. Slow emittance growth arising in a high intensity circular proton ring is studied. We assume that the beam distribution is static, and each particle moves in the filed of the static distribution. A halo is formed by the nonlinear force due to the electro-magnetic field of the beam itself. The halo, which consists of small part of whole beam, does not affect the electro-magnetic field. Particle motion is described by a single particle Hamiltonian in the field. This picture is not self-consistent for a distortion of beam distribution due to space charge force. Practical issue in J-PARC MR; the beam loss of 0.1-1% during ⇡ 10, 000 100, 000 turns.

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

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SLIDE 4

Hamiltonian and Resonances

Real issue: J-PARC MR operating point

Choice of operating point in J-PARC MR.

1 New operating point (21.3,21.4) is better than present one

(22.40,20.75) in simulations and experiments.

2 Qualitative understanding of the reasons is necessary.

Figure: Tune scan of beam loss in a space charge simulation (SCTR).

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

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SLIDE 5

Hamiltonian and Resonances

Beam loss measureemnt at new operating point (21.23,21.31)

Figure: Measured beam loss at (νx, νy) = (21.23, 21.31).

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

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SLIDE 6

Hamiltonian and Resonances

How high power is expected at new operating point

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

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SLIDE 7

Hamiltonian and Resonances Action variable representation

Hamiltonian for a particle under the space charge force

Betatron variables with action variable/angle expression. x(s) = p 2βx(s)Jx cos(φx(s)) y(s) = q 2βy(s)Jy cos(φy(s)). (1) Hamiltonian, which characterize one turn map, is separated by three parts linear betatron motion (µJ) nonlinear component of the lattice magnets (Unl) space charge potential (U). H = µJ + Unl + Usc. (2) Betatron phase advance per turn, ˜ µx = φx(s + L) φx(s) = ∂H ∂Jx = µx + ∂(Unl + Usc) ∂Jx (3)

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

7 / 36

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SLIDE 8

Hamiltonian and Resonances Action variable representation

Fourier expansion of Hamiltonian

H = µJ + U00(J) + X

mx,my6=0

Umx,my (J) exp(imxφx imyφy) (4) Tune shift, tune slope First and second terms in RHS characterize shift, spread and slope of tune. ˜ µx = ∂H ∂Jx = µx + ∂U00 ∂Jx (5) Resonance Resonance occurs, when mx ˜ µx + my ˜ µy = 2πn is satisfied at a amplitude (Jx,R, Jy,R); effect of Um is accumulated turn by turn.

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

8 / 36

slide-9
SLIDE 9

Hamiltonian and Resonances Standard model

Expansion around Resonance

  • J. L. Tennyson, AIP Conference proceedings, 87, 345 (1982).

Resonance condition mx ˜ µx(Jx, Jy) + my ˜ µy(Jx, Jy) = 2πn Above condition gives a fixed point(line) in (Jx, Jy) space for particle motion. Expansion of Hamiltonian around the fixed point U00(J) = U00(JR) + ∂U00 ∂J

  • J R

(J JR) + (J JR)t 1 2 ∂2U00 ∂J∂J

  • J R

(J JR) (6) Tune slope ∂νi ∂Jj = ∂νj ∂Ji = ∂2U00 ∂Ji∂Jj (7)

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

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SLIDE 10

Hamiltonian and Resonances Standard model

Standard Model

Resonance term around the fixed point Um(J) ⇡ Um(JR) m = (mx, my) (8) Standardized Hamiltonian H = Λ 2 P2

1 + Um(JR) cos ψ1

(9) Λ = m2

x

∂2U00 ∂J2

x

+ mxmy ∂2U00 ∂Jx∂Jy + m2

y

∂2U00 ∂J2

y

Resonance width (full width) ∆P1 = 4 r Um Λ ∆Jx = 4mx r Um Λ (10)

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

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SLIDE 11

Hamiltonian and Resonances Standard model

Standard Model

.

Figure: Relation between (Jx, φx) and (P1, ψ1).

  • K. Ohmi (KEK)

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  • Dec. 10, 2015, talk at Fermilab

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SLIDE 12

Space Charge force and its Hamiltonian

Space Charge Potential

Assume Gaussian beam in x,y,z Usc(s0, s) = λprp β2γ3 Z 1 1 exp ⇣ x(s0,s)2

2σ2

x+u y(s0,s)2

2σ2

y+u

⌘ p 2σ2

x(s0) + u

q 2σ2

y(s0) + u

du (11) x(s0, s) = p 2βx(s0)Jx cos(ϕx(s0, s) + φx(s)) + η(s0)δ(s) y(s0, s) = q 2βy(s0)Jy cos(ϕy(s0, s) + φy(s)). (12) where ϕx,y(s0, s) is the betatron phase difference between s and s0 and η is the dispersion. δ(s) is given function of s, not canonical variable. Usc(s) = I ds0Usc(s0, s) (13)

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

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SLIDE 13

Space Charge force and its Hamiltonian Tune shift and tune slope

U00

U00(Jx, Jy) = λprp β2γ3 I ds Z 1 dt p2 + tp2ryx + t (14) " 1 ewxηwy

1

X

l=1

(1)lIl/2(wx)Il(vx)I0(wy) # . where t = u/σ2

x and ryx = σ2 y/σ2 x and

wx = βxJx 2σ2

x + u .

wxη = βxJx + η2δ2 2σ2

x + u

. (15) vx = 2p2βxJxηδ 2σ2

x + u

wy = βyJy 2σ2

y + u .

(16)

  • K. Ohmi (KEK)

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  • Dec. 10, 2015, talk at Fermilab

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SLIDE 14

Space Charge force and its Hamiltonian Tune shift and tune slope

Tune shift Space Charge Potential

2π∆νx = ∂U00 ∂Jx = λprp β2γ3 I ds βx σ2

x

Z 1 ewxwy dt (2 + t)3/2(2ryx + t)1/2 [(I0(wx) I1(wx))I0(wy)] , (17)

20 40 60 80 100 20 40 60 80 100

  • 0.1
  • 0.09
  • 0.08
  • 0.07
  • 0.06
  • 0.05
  • 0.04
  • 0.03
  • 0.02
  • 0.01

∆νx Jx Jy ∆νx 20 40 60 80 100 20 40 60 80 100

  • 0.1
  • 0.09
  • 0.08
  • 0.07
  • 0.06
  • 0.05
  • 0.04
  • 0.03
  • 0.02
  • 0.01

∆νy Jx Jy ∆νy

Figure: Tune spread (∆νx,y(Jx, Jy)) due to space charge force.

  • K. Ohmi (KEK)

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  • Dec. 10, 2015, talk at Fermilab

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SLIDE 15

Space Charge force and its Hamiltonian Tune shift and tune slope

Tune footprint

  • 0.2
  • 0.15
  • 0.1
  • 0.05
  • 0.2
  • 0.15
  • 0.1
  • 0.05

∆νy ∆νx (21.39,21.43) (22.40,20.75)

Figure: Tune footprint (∆νx,y(Jx, Jy)) due to space charge force.

  • K. Ohmi (KEK)

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SLIDE 16

Space Charge force and its Hamiltonian Tune shift and tune slope

Tune slope Space Charge Potential

∂2U00 ∂J2

x

= λprp β2γ3 I ds β2

x

σ4

x

Z 1 ewxwy dt (2 + t)5/2(2ryx + t)1/2 ⇢3 2I0(wx) 2I1(wx) + 1 2I2(wx)

  • I0(wy)
  • ,

20 40 60 80 100 20 40 60 80 100

  • 25000
  • 20000
  • 15000
  • 10000
  • 5000

Uxx Jx Jy Uxx 20 40 60 80 100 20 40 60 80 100

  • 25000
  • 20000
  • 15000
  • 10000
  • 5000

Uyy Jx Jy Uyy

Figure: Tune slope (Uij = ∂2U00/∂Ji∂Jj) due to space charge force.

  • K. Ohmi (KEK)

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  • Dec. 10, 2015, talk at Fermilab

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SLIDE 17

Space Charge force and its Hamiltonian Resonance terms

Resonance terms

Umx,my (Jx, Jy) = λprp β2γ3 I ds Z 1 du p 2σ2

x + u

q 2σ2

y + u

" δmx0δmy0 exp(wxη wy)

1

X

l=1

(1)(mx+l+my)/2 I(mxl)/2(wx)Il(vx)Imy/2(wy)eimxϕximyϕy ⇤ . (18)

0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 1e-09 2e-09 3e-09 4e-09 5e-09 6e-09 7e-09 |U30| Jx Jy |U30| 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 2e-08 4e-08 6e-08 8e-08 1e-07 1.2e-07 1.4e-07 1.6e-07 1.8e-07 2e-07 |U40| Jx Jy |U40|

Figure: U30(δ = σδ) and U40(δ = 0) due to space charge force.

  • K. Ohmi (KEK)

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SLIDE 18

Lattice nonlinearity Tune shift and tune slppe

Tune shift due to lattice nonlinearity

One turn map is given by Taylar expansion of lattice elements. .

Figure: Tune spread (∆νx,y(Jx, Jy)) due to lattice nonlinearity.

  • K. Ohmi (KEK)

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SLIDE 19

Lattice nonlinearity Tune shift and tune slppe

Tune slope due to lattice nonlinearity

Tune slope is given by the one turn map.

Figure: Tune slope (∂2H00/∂J2

x , ∂2H00/∂Jx∂Jy and ∂2H00/∂J2 y ) due to lattice

nonlinearity.

The tune shift and slope due to lattice nonlinearity are one order smaller than those of space charge.

  • K. Ohmi (KEK)

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  • Dec. 10, 2015, talk at Fermilab

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SLIDE 20

Superperiodicity

.

Table: Umx,my (J) for lattice nonlinearity. U’s are evaluated at J 3rd and 4-th

  • column. The suffix, B0,B and BR means lattices without errors, lattice with

measured beta and measured beta and coupling, K.Ohmi, HB2012.

  • K. Ohmi (KEK)

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  • Dec. 10, 2015, talk at Fermilab

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SLIDE 21

Superperiodicity

J-PARC MR ring has superperiodicity of three. Resonances without mxνx + myνy = 3n is suppressed under the perfect superperidicity. It is sufficient to consider 1/3 ring. M = h exp ⇣ H(1)

00 H(1)

m ⌘i3 (19)

Figure: .Tune diagram near (νx/3, νy/3) = (7.467, 6.917) and (7.13, 7.143).

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SLIDE 22

Superperiodicity

Resonance terms under superperiodicity 3

New operating point, (νx, νy) = (21.39, 21.43), (νx/3, νy/3) = (7.13, 7.143),

0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 5e-11 1e-10 1.5e-10 2e-10 2.5e-10 3e-10 3.5e-10 (2,6,0) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 1e-10 2e-10 3e-10 4e-10 5e-10 6e-10 7e-10 8e-10 9e-10 (4,4,0) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 1e-10 2e-10 3e-10 4e-10 5e-10 6e-10 7e-10 (6,2,0) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 5e-10 1e-09 1.5e-09 2e-09 2.5e-09 3e-09 3.5e-09 (8,0,0) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 5e-11 1e-10 1.5e-10 2e-10 2.5e-10 3e-10 3.5e-10 4e-10 4.5e-10 (10,0) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 1e-11 2e-11 3e-11 4e-11 5e-11 6e-11 7e-11 8e-11 9e-11 1e-10 (1,8,1) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 1e-11 2e-11 3e-11 4e-11 5e-11 6e-11 7e-11 8e-11 9e-11 (3,6,1) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 5e-12 1e-11 1.5e-11 2e-11 2.5e-11 3e-11 3.5e-11 4e-11 (5,4,1) Jx (µm) Jy (µm)

Figure: .Resonance terms near (νx, νy) = (21.39, 21.43)

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slide-23
SLIDE 23

Superperiodicity

Resonance terms under superperiodicity 3

Present operating point, (νx, νy) = (22.40, 20.75), (νx/3, νy/3) = (7.4667, 6.9167),

0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 5e-10 1e-09 1.5e-09 2e-09 2.5e-09 3e-09 3.5e-09 (0,8,0) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 1e-10 2e-10 3e-10 4e-10 5e-10 6e-10 7e-10 (12,0,0) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 5e-10 1e-09 1.5e-09 2e-09 2.5e-09 (1,4,1) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 1e-10 2e-10 3e-10 4e-10 5e-10 6e-10 7e-10 8e-10 9e-10 1e-09 (3,2,1) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 2e-11 4e-11 6e-11 8e-11 1e-10 1.2e-10 1.4e-10 1.6e-10 1.8e-10 2e-10 (3,4,1) Jx (µm) Jy (µm) 0 10 20 30 40 50 60 70 80 90 100 10 20 30 40 50 60 70 80 90 100 1e-11 2e-11 3e-11 4e-11 5e-11 6e-11 7e-11 8e-11 9e-11 1e-10 (9,0,1) Jx (µm) Jy (µm)

Figure: Resonance terms near (νx, νy) = (22.40, 20.75).

  • K. Ohmi (KEK)

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SLIDE 24

Superperiodicity Breaking of the superperiodicity

Breaking of Superperiodicity

In real accelerator, superperiodicity is broken by various errors. Non-structure resonances appear. M = exp ⇣ H(3)

00 H(3)

m ⌘ exp ⇣ H(2)

00 H(2)

m ⌘ exp ⇣ H(1)

00 H(1)

m ⌘ (20) H(2,3)

00

+ H(2,3) m = H(1)

00 + H(1)

m + ∆H(2,3)

00

+ ∆H(2,3) m (21)

Figure: .Tune diagram near (νx, νy) = (22.40, 20.75) and (21.39, 21.43)

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SLIDE 25

Superperiodicity Beta function measurement

Beta function measurement

Beta function distortion breaks superperiodicity. Beta function and phase are measured by turn-by-turn monitor (and/or orbit response). x1, x2 : turn-by-turn positions of monitor 1 and 2, mij: transfer matrix between 1 and 2. ✓ x0

1

x0

2

◆ = 1 m12 ✓ m11 1 1 m22 ◆ ✓ x1 x2 ◆ (22) turn average of phase space position for x mode excitation ✓ βx αx ◆

1

= 1 q hx2

1ihx02 1 i hx1x0 1i2

✓ hx2

1i

hx1x0

1i

◆ (23) Betatron phase difference cos(φx,2 φx,1) = hx1x2i q hx2

1ihx2 2i

(24)

  • K. Ohmi (KEK)

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SLIDE 26

Superperiodicity Beta function measurement

Measured beta function and phase

5 10 15 20 25 30 35 40 45 200 400 600 800 1000 1200 1400 βx (m) s(m) design s112s118

  • 0.1
  • 0.08
  • 0.06
  • 0.04
  • 0.02

0.02 0.04 0.06 200 400 600 800 1000 1200 1400 ∆φ s(m) ∆φx ∆φy

Figure: Measured beta function and phase for shot 112 (x) and 118 (y).

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slide-27
SLIDE 27

Superperiodicity Beta function measurement

Space charge induced resonances with measured beta

Integration along s in Eq.(18) is performed using measured beta and phase.

2e-08 4e-08 6e-08 8e-08 1e-07 1.2e-07 1.4e-07 1.6e-07 1.8e-07 2e-07 0 10 20 30 40 50 60 70 80 90 100 |U40| Jx (/Symbol mm 1/3 2/3 3/3 2e-09 4e-09 6e-09 8e-09 1e-08 1.2e-08 1.4e-08 0 10 20 30 40 50 60 70 80 90 100 |U301| Jx (/Symbol mm (3,0,1) (3,0,1) (3,0,1)

Figure: U301 and U40 for space charge force given by measured beta function and phase.

2e-08 4e-08 6e-08 8e-08 1e-07 1.2e-07 1.4e-07 1.6e-07 1.8e-07 2e-07 0 10 20 30 40 50 60 70 80 90 100 |U301| Jx (/Symbol mm 1/3 2/3 3/3 2e-09 4e-09 6e-09 8e-09 1e-08 1.2e-08 1.4e-08 0 10 20 30 40 50 60 70 80 90 100 |U301| Jx (/Symbol mm 1/3 2/3 3/3

Figure: U301 and U40 for space charge force in the design lattice.

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slide-28
SLIDE 28

Superperiodicity Beta function measurement

Lattice magnets induced resonances with measured beta

Lattice nonlinearity is factorized in each super period (SUP). M(sup) =

N1

Y

i=0

M(si+1, si)e:HI (si): = exp ⇣ H(sup)

00

H(sup) m ⌘ , (25) M(si+1, si) = V 1(si+1)Ui+1,i∆UiV (si) (26) = V 1(si+1)V0(si+1)M0(si+1, si)V 1 (si)∆UiV (si)

Figure: Real and imaginary part of H40 for lattice nonlinearity in first SUP. Measured beta and phase are contained in V and ∆U in Eq.(26).

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slide-29
SLIDE 29

Simulation using the resonance Hamiltonian Without Synchrotron Motion

Integration of the resonance Hamiltonian

Simulation for emittance growth can be done using the resonance (Fourier expanded) Hamiltonian. H = µxJx + µyJy + U0(Jx, Jy) +Um,c(Jx, Jy) cos mφ + Um,s(Jx, Jy) sin mφ. (27) where mφ = mxφx + myφy. Symplectic transformation for above Hamiltonian is expressed by ¯ φi = φi + ∂U0 ∂Ji + ∂Um,c ∂Ji cos mφ ∂Um,s ∂Ji sin mφ Ji = ¯ Ji mi(Um,c sin mφ Um,s cos mφ). (28) where ¯ J and ¯ φ are those after the transformation, and Um’s are function of ¯ Ji and φi. Second equation of Eq.(28) is implicit relation.

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slide-30
SLIDE 30

Simulation using the resonance Hamiltonian Without Synchrotron Motion

Simulation without synchrotron motion

Figure: Phase space trajectory for the model map with U40. No synchrotron

  • motion. Left and right plots correspond to tune (22.40,20.75) and (21.39,21.43),

respectively.

Analytical estimate of the resonance width agrees well ∆Jx = 4 s Um ∂2U00/∂J2

x

= 4 r 107 104 = 12 ⇥ 106m = 12µm (29)

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slide-31
SLIDE 31

Simulation using the resonance Hamiltonian With Synchrotron Motion

Simulation with synchrotron motion

Beam charge density depends on z. The resonance structure modulates due to synchrotron oscillation. λ(z, s) = Np p 2πσz exp ✓ z(s)2 2σ2

z

◆ (30) z = z0 cos(µss/L) = z0 cos(µsnturn) (31)

Figure: Phase space trajectory for the model map with U40. Synchrotron tune, νs = 0.002, z0 = σz. Left and right plots correspond to tune (22.40,20.75) and (21.39,21.43), respectively

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slide-32
SLIDE 32

Simulation using the resonance Hamiltonian With Synchrotron Motion

Emittance growth, diffusion of J

Initializing δ(J J0), uniform φ, calculate evolution of spread of J.

0.5 1 1.5 2 2.5 3 3.5 0 100 200 300 400 500 600 700 800 900 1000 ∆J turn 2Jx=10um 20um 30um 40um 60um 1 2 3 4 5 6 7 0 100 200 300 400 500 600 700 800 900 1000 ∆J turn 2Jx=10um 20um 30um 40um 60um

Figure: Diffusion of J. Left is for no synchrotron moiton. Right is for Synchrotron tune, νs = 0.002, z0 = σz.

Diffusion of J with synchrotron motion is larger than those without synchrotron motion. All particles Jx < 40µm diffuse for finite νs, while limited particles Jx = 30 and 40 have large ∆J, but not diffusive.

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slide-33
SLIDE 33

Simulation using the resonance Hamiltonian With Synchrotron Motion

Simulation under broken superperiodicity using measured beta

Preliminary, only space charge resonances are taken into account. Very clean phase space. Probably, this result is too clean compare with beam loss experience in J-PARC MR. Resonances due to lattice nonlinearity may dominate.

Figure: .Phase space trajectory for the model map based on measured beta.

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slide-34
SLIDE 34

Summary

Summary

Emittance growth based on chaos near resonances is discussed. Tune shift and slope for space charge and lattice is evaluated. Resonance terms for space charge and lattice is evaluated. Beta function, phase and x-y coupling have been measured in J-PARC MR turn by turn monitors. Resonance terms are evaluated by the measured beta and phase. Resonance fixed point and width are determined by the tune slope and resonance strength. Simulation of a model based on the tune slope and resonance strength is being performed. Emittance growth is evaluated by combination with Synchrotron motion The results are preiminary yet for the emittance growth based on measured beta. Simulations for Multi-resonances will be performed.

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

33 / 36

slide-35
SLIDE 35

Summary

The End

Thank you for your attention

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

34 / 36

slide-36
SLIDE 36

Summary

Canonical Transformation to Resonance base

Generating function for the canonical transformation F2(P, φ) = (Jx,R + mxP1 + mx,2P2)φx + (Jy,R + myP1 + my,2P2)φy (32) Resonance base (choose mx,2 = 0, my,2 = 1) P1 = Jx Jx,R mx ψ1 = mxφx + myφy (33) P2 = (Jy Jy,R) my mx (Jx Jx,R) ψ2 = φy Hamiltonian, U00 U00 ⇡ Λ 2 P2

1

Λ = m2

x

∂2U00 ∂J2

x

+ mxmy ∂2U00 ∂Jx∂Jy + m2

y

∂2U00 ∂J2

y

(34)

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

35 / 36

slide-37
SLIDE 37

Summary

Newton Raphson method for Symplectic integration

To solve ( ¯ J, ¯ φ), Newton-Raphson method is used. fx = ¯ Jx Jx mx(Um,c sin mφ Um,s cos mφ) = 0 fy = ¯ Jy Jy my(Um,c sin mφ Um,s cos mφ) = 0. (35) Iteration of Newton method is expressed by ✓ ¯ Jx ¯ Jy ◆

n+1

= ✓ ¯ Jx ¯ Jy ◆

n

F 1 ✓ fx fy ◆

n

. (36) where F is Jacobian matrix for fi; Fij = ∂fi/∂Jj, i, j = x, y.

  • K. Ohmi (KEK)

Space charge on measured beta

  • Dec. 10, 2015, talk at Fermilab

36 / 36