Space Charge - CERN · Space Charge Luigi Palumbo Università di Roma "La Sapienza" and LNF-INFN...
Transcript of Space Charge - CERN · Space Charge Luigi Palumbo Università di Roma "La Sapienza" and LNF-INFN...
Space ChargeLuigi Palumbo
Università di Roma "La Sapienza"and LNF-INFN
CAS, 25 May 2005CAS, 25 May 2005
EQUATION OF MOTION
The motion of charged particles is governed by the Lorentz force :
( ) ( )BvEFv ext
e.m. ×+== edt
md γ
Where m is the rest mass, γ the relativistic factor and v the particle velocity
Charged particles are accelerated, guided and confined by external electromagnetic fields.
Acceleration is provided by the electric field of the RF cavity
Magnetic fields are produced in the bending magnets for guiding the charges on the reference trajectory (orbit), in the quadrupoles for the transverse confinement, in the sextupoles for the chromaticity correction.
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SELF FIELDS AND WAKE FIELDS
There is another important source of e.m. fields : the beam itself
Direct self fields
Space Charge
Image self fields
Wake fields
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These fields depend on the current and on the charges velocity.
They are responsible of many phenomena of beam dynamics:
• energy loss
• energy spread and emittance degradation
• shift of the synchronous phase and frequency (tune)
• shift of the betatron frequencies (tunes)
• instabilities.
(wake-fields)
CAS, 25 May 2005CAS, 25 May 2005
Fields of a point charge with uniform motion
o
z
x,x’
y
o’
z’
y’
v
q
0
4 3
=′′
′=′
BrrqE
or
rr
πε
vt is the position of the point charge in the lab. frame O.
• In the moving frame O’ the charge is at rest• The electric field is radial with spherical symmetry• The magnetic field is zero
34 rzqE
oz
′
′=′
πε34 ryqE
oy
′
′=′
πε34 rxqE
ox
′
′=′
πε
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Relativistic transforms of the fields from O’ to O
)/(
)/(
)(
)(2
2
cEvBB
cEvBB
BB
BvEE
BvEEEE
yzz
zyy
xx
yzz
zyy
xx
′+′=
′−′=
′=
′−′=
′+′=
′=
γ
γ
γ
γ
( )
[ ] )(
)(
1/22222
2/1222
zyvtxr
zzyy
vtxxzyxr
++−=′
=′=′
−=′
′+′+′=′
γ
γ
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[ ] 2/322223)(
)(44 zyvtx
vtxqrxqEE
ooxx
++−
−=
′
′=′=
γ
γπεπε
[ ] 2/322223)(44 zyvtx
yqryqEE
ooyy
++−=
′
′=′=
γ
γπεπε
γ
[ ] 2/322223)(44 zyvtx
zqrzqEE
oozz
++−=
′
′=′=
γ
γπεπε
γ
[ ] 2/32222
4 zyx
rqEo ++
=γ
γπε
rrThe field pattern is moving with the charge and it can be observed at t=0.
The fields have lost the spherical symmetry but still keep a symmetry with respect to the x-axis.
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t=0
x
y
z
rθ
θ
θ2222 sin
cos
rzy
rx
=+
=( ) 32/322
2
sin1
4 r
rqEo
rr
θβ
γπε −
=
γ >>1γ≠0γ=0
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B is transverse to the motion direction
2
2
/
/
0
cvEB
cvEB
B
yz
zy
x
=
−=
=
2cEvBrrr ×
=⊥
γ→∞
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Two charges in the rest frame O’
q
q
241
rqqF
or πε
=′
2411
rqqFF
orr γπεγ
=′=
Two charges in the laboratory frame O
Relativistic transform
Lorentz force
241)()( 2
2rqqEqEEqvBEqF
orrrrr γπεγ
βϕ ==−=−=
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It is the net effect of the Coulomb interactions in a multi-particle system.
Space Charge Regime dominated by the self field produced by the particle distribution.
Collective Effects
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What do we mean with “space charge”?
Debye Length λD
Φ
r r ( )=
Cr
C =e
4πεo
real uniform
The particle distribution around a test particle will deviate from the continuous distribution.
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The effective potential of a test charge can be defined as the sum of the potential of the uniform distribution and a “perturbed” term.
( ) Drp e
rCr λ/−=Φ
r
λD =εokBTe2n
kB= Boltzman constantT = TemperaturekB T = average kinetic energy of the particlesn = particle density (N/V)
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The effective interaction range of the test charge is limited to the Debye length
λλDD
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Smooth functions for the charge and field distributions can be used as long as the Debye length remains small compared to the particle bunch size
Longitudinal Electric field of a uniform charged cylinder
1.498 1.499 1.501z[ m]
-200000
-100000
100000
200000Ez [ V/ m]<z>=1.50 [ m]
As computed by a multi-particle tracking code
Analytical expression
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Space charge of a relativistic cylindrical distribution
L
RCylindrical finite bunch, uniformly charged,With circular cross section
-0.002 0.002 0.004 0.006
1
2
3
4
5Er
-0.002 0.002 0.004 0.006
-1.5
-1
-0.5
0.5
1
1.5EzTransverse electric field at r = a
Longitudinal electric field at r = 0
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Relativistic Uniform Cylinder
εoE ⋅ dS = ρdV∫∫
arfor 22 2 ≤==
vaIrrEoo
r πεερlrErl ro
22 ρπεπ =
J =I
πa2ρ =I
πa2va
Gauss’s law Linear with r
rEc
B βϕ =
Ampere’s law ∫ ∫ ⋅=⋅ dSJdlB oµ
arfor 22 2 ≤==
aIrJrB o
o
πµµ
ϕJlrlB oµϕ =2
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)/(2 mCao ρπλ =
2
2
2
)()(B
2
)(
ar
crE
cr
arrE
arfor
o
or
o
or
=
=
=
<
πεβλβ
πελ
θ
2)/()( arr oλλ =
)()/(0
2
2
AcaJImAcJ
λβπ
ρβ
==
=
The Lorentz Force
( ) ( ) 2222
21
areeEEecBEeF
o
orrrr γπε
λγ
ββ ϑ
==−=−=
• has only radial component
• is a linear function of the transverse coordinate
The attractive magnetic force, which becomes significant at highenergy, tends to compensate the repulsive electric force.
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Longitudinal Space Charge Forces
In order do derive the relationship between the longitudinal andtransverse forces inside a beam, let us consider the case of cylindrical symmetry and ultra-relativistic bunches. We know that a varying magnetic field produces a rotational electric field:
∫∫ ⋅∂∂
−=⋅S
dSt
nBdlE
z+∆zzWe choose as path a rectangle going through the beam pipe and the beam, parallel to the axis.
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drrBt
z
drzrEzzbEdrzzrEzzrE
b
r
b
rrz
b
rrz
)(
),(),(),(),(
∫
∫∫
∂∂
∆−=
=−∆−∆++∆
θ
[ ]
[ ]drzrvBzrEz
zbEzrE
drzrvBzrEz
zbEzrE
drt
zrBz
zrEzbEzrE
b
rrzz
b
rrzz
b
r
rzz
∫
∫
∫
−∂∂
+=
−∂∂
+=
∂∂
−∂
∂+=
),(),(),(),(
),(),(),(),(
),(),(),(),(
θ
θ
θ
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∫∂∂
−+=b
rrzz drzrE
zzbEzrE ),()1(),(),( 2β
where (1-β2)=1/γ2. For perfectly conducting walls Ez=0.
∫∂∂
=b
rrz z
12γ
drzrEzrE ),(),(
b
rUniform beam in a circular p.c. pipe.
zz
ab
arezrFz ∂
∂+−
−=
)()ln21(4
),( 2
2
20
λγπε
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r.m.s. emittance
γx 2 + 2αx ′ x + β ′ x 2 = εrms
x2 = βεrms and ′ x 2 = γεrms α = −′ β
2= −
12εrms
ddz
x2 = −x ′ x εrms
εrms = x2 ′ x 2 − x ′ x 2
x
x’
xrms
x’rms
γβ −α 2 = 1
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Emittance degradation
Longitudinal correlation along the bunch induced by e.mnon linear e.m. fields
x
x’
x
x’
RF fields, solenoidal fields, space charge, wake fields
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Equation of motion in a drift space:
γm d2rdt2 =
eEr
γ 2 =eI
2πγ 2εoa2v
r
d2rdt2 = β 2c2 d2r
dz2
d2rdz2 =
eI2πmγ 3εoa
2v3 r =Ka2 r
K =eI
2πmγ 3εov3 =
2IIoβ
3γ 3 Generalized perveance
Io =4πεomc3
e Alfven current
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Transport in a Long Solenoid
ks =qB
2mcβγ K ζ( )=2Ig ζ( )Io βγ( )3
0 0.0005 0.001 0.0015 0.002 0.0025metri
0.5
0.6
0.7
0.8
0.9
gg(ζ)
ζ
′ ′ R + ks2R =
K ζ( )R
==> Equilibrium solution ==>′ ′ R = 0 Req ζ( )=K ζ( )ks
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Emittance Oscillations are driven by space charge differential defocusing in core and tails of the beam
x
px
Slice Phase Space
Projected Phase Space
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Envelope oscillations drive Emittance oscillations
0 1 2 3 4 5metri
-0.5
0
0.5
1
1.5
2
envelopes
0 1 2 3 4 5metri
0
20
40
60
80
emi
R(ζ)
ε(z)
δγγ
= 0
ks =qB
2mcβγ
ε z( )= R2 ′ R 2 − R ′ R 2 ÷ sin 2ksz( )CAS, 25 May 2005CAS, 25 May 2005
BEAM DYNAMICS MODELING
RF Field + Solenoids
∆t
Space chargeOn Axis
Off Axis∆t
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Envelope equation (linear fields)On axis
Space charge
3
2
322 14),,()(
xxAE
mexkkxx
thn
xssscx
solrf
+=+++
γεξ
γββγ &&&
3
2
322 14),,()(
yyAE
meykkyy
thn
xssscx
solrf
+=+++
γεξ
γββγ &&&
RF fieldSolenoid field
CAS, 25 May 2005CAS, 25 May 2005
CODES used for simulations of Space Charge Effects
PARMELA, ASTRA
Multi-particle tracking code, includes space charge but not wake fields
HOMDYN
Relies on a multi-envelope model based on the time dependent evolution of a uniform bunch
CAS, 25 May 2005CAS, 25 May 2005
Effects of conducting or magnetic screens
Let us consider a point charge q close to a conducting screen.
The electrostatic field can be derived through the "image method". Since the metallic screen is an equi-potential plane, it can be removed provided that a "virtual" charge is introduced such that the potential is constant on the screen
q q - q
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A constant current in the free space produces circular magnetic field.
If µr≈1, the material, even in the case of a good conductor, does not affect the field lines.
I
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For ferromagnetic type, with µr>>1, the very high magnetic permeability makes the tangential magnetic field zero at the boundary so that the magnetic field is perpendicular to the surface, just like the electric field lines close to a conductor.
I I I
In analogy with the image method we get the magnetic field, in the region outside the material, as superposition of the fields due to two symmetric equal currents flowing in the same direction.
CAS, 25 May 2005CAS, 25 May 2005
Time-varying fields
Static electric fields vanish inside a conductor for any finite conductivity, while magnetic fields pass through unless of an high permeability. This is no longer true for time changing fields, which can penetrate inside the material only in a region δw called skin depth. Inside the conducting material we write the following Maxwell equations:
∂∂
+=×∇
∂∂
−=×∇
tDJH
tBE
B = µHD = εEJ = σE
Copper σ = 5.8 107 (Ωm)-1
Aluminium σ = 3.5 107 (Ωm)-1
Stainless steel σ = 1.4 106 (Ωm)-1 .CAS, 25 May 2005CAS, 25 May 2005
Consider a plane wave (Hz,Ey) propagating in the material
02
2
2
2=
∂
∂−
∂
∂−
∂
∂
tE
t
E
x
E yyy σµεµ
( the same equation holds for Hz). Assuming that fields propagate in the x-direction with the law:
Hz = ˜ H oeiωt−γx
Ey = ˜ E oeiωt−γx
(γ 2 + εµω 2 − iωµσ ) ˜ E oeiωt−γx = 0
We say that the material behaves like a conductor if σ>>ωε thus:∆w
Ey
xHz
2)1( σµεγ i+≅
CAS, 25 May 2005CAS, 25 May 2005
Fields propagating along “x” are attenuated. The attenuation constant measured in meters is called skin depth δw:
δw
ωσµγδ 2
)(1
=ℜ
≅w
∆w
The skin depth depends on the material properties and the frequency.Fields pass through the conductor wall if the skin depth is larger than the wall thickness ∆w. This happens at relatively low frequency.
At higher frequency, for a good conductor δw<< ∆w and both electric and magnetic fields vanish inside the wall.
)(66.6 cmfw ≅δFor the copper
For a pipe 2mm thick, the fields pass through the wall up to 1 kHz. (Skin depth of Aluminium is larger by a factor 1.27)
CAS, 25 May 2005CAS, 25 May 2005
• compare the wall thickness and the skin depth (region of penetration of the e.m. fields) in the conductor.
• If the fields penetrate and pass through the material, they caninteract with bodies in the outer region.
• If the skin depth is very small, fields do not penetrate, the electric filed lines are perpendicular to the wall, as in the static case, while the magnetic field line are tangent to the surface.
I -II -I
CAS, 25 May 2005CAS, 25 May 2005
Circular Perfectly Conducting Pipe
(Beam at Center)In the case of charge distribution, and γ→∞, the electric field lines are perpendicular to the direction of motion. The transverse fields intensity can be computed like in the static case, applying the Gauss and Ampere laws.
λ(r) = λora
2
; ErS
∫ (2πr)∆z =λ(r)∆z
εo
Er =λ(r)∆z2πεor
; Bθ =βc
Er
Er(r) =λo
2π εo
ra2 ; Bθ (r ) =
λoβ2πεoc
ra2
F⊥ (r) = e(Er − βc Bθ ) =eγ 2 Er
CAS, 25 May 2005CAS, 25 May 2005
• Due to the symmetry, the transverse fields produced by an ultra-relativistic charge inside the pipe are the same as in the free space.
• For a distribution with cylindrical symmetry, in the ultra-relativistic regime, there is a cancellation of the electric andmagnetic forces.
• The uniform beam produces exactly the same forces as in the free space.
• This result does not depend on the longitudinal distribution of the beam. In general one has to consider the local charge density λ(z)
CAS, 25 May 2005CAS, 25 May 2005
Parallel Plates (Beam at Center)
2hq
q
q
-q
-q In some cases, the beam pipe cross section is such that we can consider only the surfaces closer to the beam, which behave like two parallel plates. In this case, we use the image method to a charge distribution of radius a between two conducting plates 2h apart. By applying the superposition principle we get the total image field at a position yinside the beam.
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Eyim(z ,y) =
λ(z )2π εo
(−1)n
n=1
∞
∑ −2y2nh( )2 − y2
≅λ (z)
4π εoh2
π 2
12y
yEy
im(z ,y) =λ(z )2π εo
(−1)n
n=1
∞
∑ 12nh + y
−1
2nh − y
Where we have assumed h>>a>y.
For d.c. or slowly varying currents, the boundary condition imposed by the conducting plates does not affect the magnetic field.
CAS, 25 May 2005CAS, 25 May 2005
From the divergence equation we derive also the other transversecomponent:
∂∂x
Exim = −
∂∂y
Eyim ⇒ Ex
im(z ,x) =−λ(z )
4π εoh2
π 2
12x
Including also the direct space charge force, we get:
Fx(z ,x) =eλ(z )xπ εo
12a2γ 2 −
π 2
48h2
Fy(z ,x) =eλ(z )yπ εo
12a2γ 2 +
π 2
48h2
There is no cancellation of the electric and magnetic forces due to the "image" charges.
CAS, 25 May 2005CAS, 25 May 2005
Parallel Plates (Beam at Center) a.c. currents
Usually, the frequency beam spectrum is quite rich of harmonics,especially for bunched beams.
It is convenient to decompose the current into a d.c. component, I, for which δw>>∆w, and an a.c. component, Î, for which δw<< ∆w.
While the d.c. component of the magnetic does not perceives the presence of the material, its a.c. component is obliged to be tangent at the wall. For a charge density λ we have I=λv.
We can see that this current produces a magnetic field able to cancel the effect of the electrostatic force.
CAS, 25 May 2005CAS, 25 May 2005
˜ E y (z, x) =˜ λ (z)yπ εo
π 2
48h2 ; ˜ B x(z,x) =βc
˜ E y(z,x)
˜ F y(z,x) = e ˜ λ (z)yπ εoγ 2
π 2
48h2
I
-I
-I
I
I
˜ F x (z, x) =e ˜ λ (z)x
2π εoγ 21a2 −
π 2
24h2
˜ F y(z,x) =e ˜ λ (z)y2π εoγ 2
1a2 +
π 2
24h2
There is cancellation of the electric and magnetic forces !!
CAS, 25 May 2005CAS, 25 May 2005
Parallel Plates - General expression of the force
Taking into account all the boundary conditions for d.c. and a.c. currents, we can write the expression of the force as:
yxu
ughha
eFo
u
,
12242411
2 2
2
2
22
2
2
22
=
+
= λππβλπ
γεπmm
where λ is the total current, and λ its d.c. part. We take the sign (+) if u=y, and the sign (–) if u=x.
CAS, 25 May 2005CAS, 25 May 2005
Self Fields and betatron motion
Consider a perfectly circular accelerator with radius ρx. The beam circulates inside the beam pipe. The transverse single particle motion in the linear regime, is derived from the equation of motion. Including the self field forces in the motion equation, we have
d mγ v( )
dt= F ext r
r ( )+ F self r r ( )
O
ρx
y
x
z
dvdt
=F ext r
r ( )+ F self r r ( )
mγ
CAS, 25 May 2005CAS, 25 May 2005
For the single particle "transverse dynamics" we write:
( )( )
( )[ ] ( )[ ] zoxoyxxo
zxoyx
yxx
exxeyexxa
exeyexv
eyexr
ˆ2ˆˆ
ˆˆˆ
ˆˆ
2 &&&&&&r
&&r
r
ωρωρω
ρω
ρ
+++++−=
+++=
++=
For the motion along x:
( ) ( )selfx
extxxo FF
mxx +=+−
γρω 12&&
Which, with respect to the azimuthal position s=vzt becomes:
( )
( )selfx
extx
zx
xoz
FFmvx
x
xxxvx
+=+
−′′
′′+=′′=
γρ
ρω
2
222
11&&
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We assume small transverse displacements x with respect to the closed orbit, and only dipoles for bending and quadrupole to keep the beam around the closed orbit:
xx
FFFx
extxext
oext
x0=
+≈
∂∂ x<<ρx
Around the closed orbit, putting vz= βc, we get
)(1112
022 xF
Ex
xF
Ex self
xox
extx
ox β∂∂
βρ=
−+′′
=
where Eo is the particle energy. This equation expressed as function of “s” reads:
′ ′ x (s)+1
ρx2(s)
+ Kx(s)
x(s) =
1β 2Eo
Fxself (x,s)
CAS, 25 May 2005CAS, 25 May 2005
•In the analysis of the motion of the particles in presence of the self field, we will adopt a simplified model where particles execute simple harmonic oscillations around the reference orbit.
•This is the case where the focussing term is constant. Although this condition in never fulfilled in a real accelerator, it provides a reliable model for the description of the beam instabilities
x(s) = Ax cos Kx s− ϕx[ ]ax βx = Ax ⇒ βx const.
Kx(s)βx2 = 1
βx =1
µ x' =
1Kx
µ x(s) = Kx s
Qx =ωx
ωo
=1
2πd ′ s
β( ′ s )o
L
∫ = ρx Kx ⇒ Kx =Qx
ρx
2
′ ′ x (s)+ Kxx(s) =1
β 2Eo
Fxself (x)
′ ′ x ( s) +Q x
ρ x
2
x( s) =1
β 2Eo
Fxself ( x , s)
CAS, 25 May 2005CAS, 25 May 2005
Transverse Incoherent Effects
We take the linear term of the transverse force in the betatronequation:
xx
FE
xQx
xx
FzxF
x
csx
ox
x
x
csxcs
x
0
..
2
20
....
1
),(
=
=
=
+′′
≅
∂∂
βρ
∂∂
( )
−=∆⇒∆+≅∆+
xF
QEQQQQQQ
csx
xo
xxxxxxx ∂
∂β
ρ ..
2
222
22
The betatron shift is negative since the space charge forces are defocusing on both planes. Notice that the tune shift is in general function of “z”, therefore there is a tune spread inside the beam.
CAS, 25 May 2005CAS, 25 May 2005
Consequences of the space charge tune shifts
In circular accelerators the values of the betatron tunes should not be close to rational numbers in order to avoid the crossing of linear and non-linear resonances where the beam becomes unstable.
The tune spread induced by the space charge force can make hard to satisfy this basic requirement. Typically, in order to avoid major resonances the stability requires
3.0<∆ uQ
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oxooo
xx lQEa
NeQ 222
22
4 γβπερ
−=∆
Example: Incoherent betatron tune shift for an uniform electron beam of radius a, length lo, inside circular perfectly conducting Pipe
2222
..
2
2
ae
axe
xxF
o
o
o
ocs
x
γπελ
γπελ
∂∂
∂∂
==
)01 53.1 : ,01 82.2:( 4
18152
2
, mprotonsmelectronscm
er
oope
−−=πε
oxo
pexx lQa
NrQ 322
,2
γβρ
−=∆
For a real bunched beams the space charge forces, and the tune shift depend on the longitudinal and radial position of the charge.
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PS Booster, accelerate proton bunchesFrom 50 to 800 MeV in about 0.6 s. The tunes occupied by the particle are indicated in the diagram by the shaded area. As time goes on, the energy increase and the space charge tune spread gets smaller covering at t=100 ms the tune area shown by the darker area. The point of highest tune correspond to the particles which are least affected by the space charge. This point moves in the Q diagram since the external focusing is adjusted such that the reduced tune spread lies in a region free of harmful resonances.
Finally, the small dark area shows the situation at t=600 ms when the beam hasReached the energy of 800 MeV. The tune spread reduction is lower than expected with the energy increase (1/γ3) dependence since the bunch dimensions also decrease during the acceleration.
CAS, 25 May 2005CAS, 25 May 2005