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Space Charge Effects in Linacs
CERN-School High Intensity Limitations, 2015 November 2-11, 2015 Ingo Hofmann
GSI Darmstadt / TU Darmstadt
Space Charge Effects in Linacs CERN-School High Intensity - - PowerPoint PPT Presentation
Space Charge Effects in Linacs CERN-School High Intensity Limitations, 2015 November 2-11, 2015 Ingo Hofmann GSI Darmstadt / TU Darmstadt 1 Overview This lecture focuses on direct space charge p or heavy ion high intensity linacs at
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CERN-School High Intensity Limitations, 2015 November 2-11, 2015 Ingo Hofmann
GSI Darmstadt / TU Darmstadt
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energies
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GeV Average Intensity
hands-on maintenance requires beam loss < 1W/m control of beam power loss at level 10-6 for MW beam power
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Envelope dynamics with linear space charge in linear optics Multi-particle beam dynamics in idealized linear (nonlinear) optics with nonlinear space charge Multi-particle beam dynamics in optics with random errors
design verification of design beam halo and loss prediction Analytical basis: Reiser’s book
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bunches usually close to spherical (within factor of 2) image charges usually negligible (pipe far away) forces Ex,y,z = linearly increasing with amplitudes in uniform bunch in non-uniform bunch non-linear Ex,y,z not negligible major source of ε growth z x
Ez – non-uniform density Ez – uniform density
z y, x,
axi
with ellipsoid uniform for
z y x z x z y x x
long)
approximation - if emittances constant!
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3 z 2 z ' ' 3 y 2 y ' ' 3 x 2 x ' '
y x z z z z y x y y y z y x x x x
5 20 qN K : parameter charge space xx'
x : emittances rms 5 / : sizes beam rms
2 3 2 2 2 2 2 x , , , ,
mc r a
z y x z y x
γ β πε ε = = =
numerous studies: Struckmeier and Reiser, Part. Accel. 14 (1984) ..............Li and Zhao, PRSTAB 17 (2014)
8 Linac:
8 GeV 2 MW H- proton driver @ FNAL
Circular tune diagram
Linac:
− nonlinear − periodically varying
Circular:
− avoid or compensate
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Proposal of a sc 8 GeV H- proton driver for Fermilab (Project X)
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F/2 – O – D – O – F/2 with symmetric RF gaps
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k0xy 0 weaker focusing beam size grows more space charge dominated although absolute space charge force weaker!
k0xy weakened kxy/k0xy more depressed !! kxy kz
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50 100 150 200 250 10 20 30 40 50 60 70 80 90 100
Losses, Rad/C BLM Position, m
H
SCL Losses for Production Optics, 30 mA
5 10 15 20 25 30 35
1 2 3 4 5 6 7
B, T/m SCL Quad Index
Design Minimal Losses 03/04/2011
source: J. Galambos et al.
Beam Stripping of H- (Valeri Lebedev, FNAL)
losses were reduced to an acceptable level.
dominated
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deviation from stable equilibrium = „mismatch“
instability
small deviations runaway
resonant excitation
periodic kick
Beam: potential from magnets/RF and self-consistent electric field all 3 involve resonant mechanisms – also in linac!
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− http://irfu.cea.fr/Sacm/logiciels/.
− model halo particles accurately far away from core
− ignore image charges – direct space charge dominant
− worry about loss at level 10-6
− effect on beam loss
− noise needs to be checked
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rms emittances
initialization 5% growth
kx,y,z
initial mismatch crossing 2kxy-2kz=0 90 degree resonance crossing 6kxy=3600
k0x,y,z
Initial density profile mismatch
distribution
< 1 betatron period) 17
1. Structure resonances
charge force resonance condition
2. Anisotropy
difference between degrees of freedom
emittances (rings: “Montague resonance”)
“90 degree” stopband envelope instability”
Distinction instability – resonance sometimes confused Not all equally serious
driven by rms mismatch periodic force from space charge
− 1D: Wangler et al., IEEE Trans. Nucl. Sci. NS·32, 2196 (1985) − 3D: Hofmann and Struckmeier, Part. Accel. 81, 69 (1987)
charge limit (k/k00) (self-consistent solution including non-parabolic space charge potential)
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emittance dominated moderate extreme space charge limit k/k00 k/k0~1 space charge (vanishing emittance – “cold” beam)
matched density profiles (schematic – Gaussian distribution):
increasing space charge effect profile flattening
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z y x
, , matched
2 initial 2
with same charge and same rms size
the extra electrostatic energy ∆W transforms into additional rms emittance
2 / 1 2 2
initial final initial final
see: Hofmann and Struckmeier, 1987
case 1
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~ good agreement! phase space plot suggests a space charge octupole as driving force! Analytical estimate in spherical approximation and assuming Ufinal=0:
k/k0 Uinitial ∆ε/ ∆ε/ ∆ε/ ∆ε/ε ε ε εinitial
0.5 0.06 (WB) 3 % 0.25 “ 13 % 0.5 0.26 (Gauss) 12 % 0.25 “ 51 %
(k0z=850)
r.m.s. envelope equations
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European Spallation Source 2.5 GeV 5 MW p linac
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rms emittances
90 degree stopband
k0x,y,z symbolic nomenclature: Linac Circular machine Envelope instability 2kxy~1800 2Qxy~½ 4th order resonance*) 4kxy~3600 4Qxy~1 Do we expect 2nd order envelope instability
Let experiment decide!
*) driven by space charge pseudo-octupole
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Avoid Mathieu instability at k0 = 1800 x’’ = (a - 2 q cos2φ)x =0
source: Reiser book quasi-periodic with increasing amplitude
2:1 structure resonance :
Resonance or instability?
instability with exponential growth
structure
structure = basic FODO cell
2 1 / = = = m n k m n
change length at double freuquency
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single particle k 900 per focusing period perturbed envelope “k” ~ 1800 per period also 2:1 relationship particles driven exponentially unstable by envelope perturbation
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Main question:
2kx ∼ 1800 = envelope instability 4kx ∼ 3600 = fourth order resonance (driven by
space charge octupole in non-uniform beam)
both may occur! - experiment should decide which one dominates!
16 cells!
4-th order!
evidence that dominance of 4th order resonance over 2nd order instability?
to be published in PRL, Nov. 2015
27 k0xy =950 kxy =800 Gaussian bunch
envelope instability at 2kx ∼ 1800 takes over and strongly exceeds 4-th order!
UNILAC-exp. cells density in x over 500 cells cells
agrees well with UNILAC- experiment (~30% rms
emittance growth over 16 cells)
evidence that envelope instability can dominate over 4th order in a longer system
4-th order resonance 4kx ∼ 3600
28 kxy: 76 90 stopband > 50...100 cells =envelope instability < 50 cells=4th order resonance
stop-band width ~ ∆ ∆ ∆ ∆k (space charge tune shift)
UNILAC kxy/k0xy=0.85
k0xy=900
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particle resonance condition!
Might be observable (which one?) also in SIS 18 (12 Sup-Per) for Qy 3 k0xy 900 (possibly by bunch compression with Q0y=3.2)
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Instabilities require:
driving force (space charge multipole):
normally resonance condition needed resonant instability theoretically they exist in all orders – practically may be limited (mixing) no justification on usual resonance diagram
Resonances:
for space charge multipoles present initially with non-uniform density multipole might grow further – self-consistent treatment - a mix of resonance and instability theoretically in all orders – mixing!
discussed in 2015 PRL paper
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x´ x x x´
cell 61 cell 60
Found “third order instability”
instability − 2 periods per lattice period − “1800” parametric 2:1 instability
sextupole − not a priori present in beam − grows with exponential growth from noise level − essentially different from a 3rd
circular machine !
Linac Circular machine 3rd order instability 3kxy~1800 3Qxy~½
+ 1800
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Waterbag Gaussian Much weaker for Gaussian distribution
− ignorable − due to Landau damping?
6kxy~3600 8kxy~3600
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rms emittances
coupling resonance with exchange of transverse – longitudinal emittances
k0x,y,z Linac Circular machine Coupling resonance 2kxy-2kz~0 2Qx-2Qy~0 (“Montague”)
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How can emittance exchange happen?
x x z z x z
T=1:
“Equipartitioned beam”:
3D: PIC-simulations
2D: Vlasov-theory + PIC “envelope” “sextupolar” “octupolar”
density perturbations
35 t i n th y y x x i i i i i
ω
1 n 1 1 2 1 1 1 1 2 2 2 2 2 2 2 1 2 1 2 1 2 1 2 1
− =
Theory see: Hofmann, Phys. Rev. E 57, p.56 (1998)
requires Vlasov-Poisson equations: analytical dispersion relations for orders n=2, 3, 4
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stop-band width:
z x z
k ∆ − = Θ 1 2 3 ε ε
360 1
1 z x z ex
N σ ε ε ∆ ⋅ − ≈
−
Nex= # of betatron periods needed for exchange
2kz - 2kxy ~ 0
2kz - kxy ~ 0 kz - 2kxy ~ 0
kz / kxy kxy / k0xy
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European HIPPI Project (2003-08)
(High Intensity Pulsed Proton Injector)
Strengthen basis for future high intensity linacs (CERN-SPL, FAIR p injector...)
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kz/kx
Experimental Evidence of Space Charge Driven Emittance Coupling in High Intensity Linear Accelerators
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− unnecessary constraint on design freedom
− all “white” zones “good” − helps avoid exchange between εz and εxy (intensity dependent design uncertainty!) − avoids a danger of halo coupling
x x z z x z
kz / kxy kxy / k0xy
T=1 2kz - 2kxy ~ 0
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x-y-halo from 900 stopband (or from errors!) couples into longitudinal plane risk loss out of bucket during acceleration
coupling resonance 90 degree stopband
99.9% emittances rms emittances
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Project X, P. Ostroumov. 2008
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H.C. Liu, HB2014
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2:1 resonance core:particle mismatch- factor MM=1.3
rms emittance
99.9% emittance (halo) 99.9% emittances rms emittances
cell 39 cell 261
2nd order resonance
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Maximum halo little dependent on
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Error study:
to avoid activation
source: S. Peggs et al., ESS TDR 2012
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− sources of emittance and halo growth − beam dynamics in principle on solid ground − in practice very transient situations
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− sometimes compromise
− statistical studies (questions open) − more to understand theoretically