analysis of the electron pinch during a bunch passage
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Analysis of the Electron Pinch during a Bunch Passage. Elena Benedetto , Frank Zimmermann CERN. Contents. Analytical calculation of the electron density evolution during the passage of a proton bunch through the electron cloud ( linear force approximation ) - PowerPoint PPT PresentationTRANSCRIPT
Analysis of the Electron Pinch during a Bunch Passage
Elena Benedetto, Frank Zimmermann
CERN
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 2
Contents
• Analytical calculation of the electron density evolution during the passage of a proton bunch through the electron cloud (linear force approximation)
• Expression for the tune shift experienced by the protons into the bunch.
• Simulations: extension to non-uniform, e.g. Gaussian, transverse beam profiles, which give rise to non-linear forces on the electrons.
• Estimation of the tune spread from the simulations results.
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 3
Electron Pinch along the bunch
The electrons are accumulated around the beam center during the bunch passage (pinch)
The aim is trying to understand the mechanism of the slow emittance growth, that is probably caused by the tune shift and tune spread due to the electron pinch.
For this reason we compute the electron cloud density evolution during a bunch passage.
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 4
Highlights of the analytical calculations
Equation of motion of an electron in the bunch
potential
Time evolution of the electron density
Tune shift experienced by the protons
Linear force approximation
via Liouville theorem
Uniform Gaussian
For any longitudinal bunch profile
Initially Gaussian electron
distribution
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 5
Electron density evolution• Electron distribution in the phase space (the density is obtained
by integrating in the velocities). • In the linear force approximation, the horizontal and vertical
planes are uncoupled → factorization
tyytxxtyyxx yx ,,,,,,,,
20
20
20
20
'22
0000 '2
0,,,,
xx
exx eexxtxx
• Liouville Theorem + assumption of Initial Gaussian Distribution
• (x0, x’0) are obtained as a function of (x, x’) by inverting the solution of the Eq. of motion xxfxx ,, 00
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 6
Equation of motion of an electron in the bunch potential (1)
• Bunch distribution:
2
2
222
)(~
,~ r
r
r
bb e
zezr
z)(nσc
t z 1
3
22
0
22
2
22
2
12
,rm
le
r
te
rm
ltreE
dt
rdm
e
r
b
ebe
r
• We consider t=0 when the bunch enters into the cloud:
• Equation of motion ( the Electric field is obtained via Gauss Theorem):
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 7
• Solution in the form:
Equation of motion of an electron in the bunch potential (2)
02 xtωx e 2
22
r
ebe
crtt
• Horizontal component of the Eq.of motion + approximation of linear force (r«r):
00
00
)()(
)()(
xtxtx
xtxtx
1)()()()( tttt
• It can be inverted and inserted into the expression of the phase space density.
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 8
Tune shift
• The tune shift experienced by the protons (as a function of r and z) is:
r
zrezrEe
02
),(~
),(~
x
C
x ksdsQ )(41 x
E
cm
ek xe
px
,
2
txxxdtxn xx ,,,
• The tune shift is obtained from the electron density, which is computed by integrating the phase space distribution:
tyntxntrn yx , ,,
• Where Ee is the field produced by the electrons is (→from Gauss theorem):
r
e drrzrnzr0
'),'(~2),(~
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 9
Longitudinal Uniform Profile (1)
2
22
2 0
r
eb
e
e
cr
xx
xCsxtxtxx
xS
Cxtxtxx
eeee
ee
ee
cossin
sin1
cos
0
0
22
0222
0
220
2220'2
22
2
'2,,,,
CS
etyntxntyxn
e
CeS
re
eeyx
• Eq. of motion → harmonic oscillator :
• The electron density is:
• The solution can be easily inverted:
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 10
• The maximum tune shift is inversely dependent on the electron initial temperature:
• For ’0 « e it goes periodically to very high values when
20
2
'
1
4ˆ
epe
x
rLQ
20
220
22
22
20
22
20'
220
2 '21
1
1
4),(
SC
r
C
rLzrQ
e
e
eC
S
pex
• The tune shift is:
Longitudinal Uniform Profile (2)
0cos tC eKeep in mind
that this is only valid for the transverse linear force
approximation !!!
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 11
• Eq. of motion:
• We look for a solution in the form:
• WKB approximation:
• The general solution can also be written as:
General longitudinal distribution (1)
; 0)(2 xtx e2
22 )(
r
ebe
crt
)()()( tiSetAtx
ee
e
e
e
2,2
3
)()(
)(
1)(
ttS
tStA
e
)()(
)(cos)(
)( 21 tsinSt
ctS
t
ctx
ee
t
e dtttS0
)()(
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 12
General longitudinal distribution (2)
• c1 and c2 are determined by the initial condition, so we obtain again a solution of the form:
• that can be inverted in order to get:
• The electron density is:
• And the tune shift:
xtdtcx
xtbxtax
)()(
)()(
0
0
)(2
2
)(2),( tD
r
etD
trn ee
2
022
02 ')()()( tbtdtD
4
0
2
4
31
4),(
r
OD
r
D
rLzrQ pe
x
00 ,, xxLxx
1)()()()( tctbtdta
In particular, we find the
expression of D(t) for a
longitudinal Gaussian
distribution
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 13
Vertical position vs. time for 6 electrons at different start amplitude, from 0.5b to 3b : linear force approximation (left) and Gaussian
transverse profile (right). Gaussian bunch shape in z.
Simulations: Linear and Gaussian force (2)
z/z z/z
vert
ical
pos
ition
[m
]
vert
ical
pos
ition
[m
]
(Parametres of LHC @ inj)
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 14
Electron density vs. time at the centre of the pipe, during the passage of a bunch, assuming a linear transverse force (Left) and a Gaussian transverse beam profile (Right). In green, the analytical results. A Gaussian bunch profile is assumed in z.
Simulations: Linear and Gaussian force (1)
z/zz/z
00
(The head of the bunch is on the right)
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 15
Snap shot of radial distribution (∙r) at 4 different times during
the bunch passage: linear force approximation (left) and Gaussian transverse profile (right).
Simulations: Linear and Gaussian force (3)
r/b r/b
ec-d
ensi
ty[
a.u
.]
ec-d
ensi
ty[
a.u
.]
z=- 3z
z=- 1.5z
z= 0z
z= 3z
z=- 3z
z=- 1.5z
z= 0z
z= 3z
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 16
Density enhancement during the bunch passage (non linear force)
Ec-density vs. Time, during the passage of a Gaussian bunch
Inside the bunch the density enhancement is about a factor 50.
z/z
/0
t0
t1 t3
t2
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 17
Horizontal phasespace at different time step:
t0 = when the bunch enters into the cloud (z=-3z)
t1 = first peak
t2 = first valley
t3 = last peak
t0 t1
t3t2
Density enhancement during the bunch passage (non linear force)
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 18
Estimated incoherent tune shift from the simulations (non linear force)
• The density enhancement at the centre of the bunch is about a factor ~ 50.
• A simple evaluation of the tune shift gives the value:
0
2
50
2
e
pe
px n
rLn
rLQ
~ 0.13
3110 106 mne
Where the unperturbed electron density is:
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 19
• The tune shift expected from an unperturbed cloud is about ~ 0.0025.
• The spread of the tune footprints computed via frequency map analysis from HEADTAIL simulations is ~20 times larger
• In our estimate we got ~50 times larger
Courtesy Papaphilippou
Estimated incoherent tune shift from the simulations (non linear force)
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 20
Summary• Analytical approach to investigate the cause of a
slow emittance growth due to the tune shift and tune spread from the electron pinch.– Analytical expression for the ec-density evolution
along the bunch and for the tune shift induced on the protons (linear force approximation)
– Numerical extension to non-linear force effects.
• The simulations (with the parameters of LHC @ inj.) show that the density enhancement inside the bunch is about a factor 50.– First estimation gives a tune spread of Q ≈ 0.13 (for
an initial ec-density of 6e11 m-3.
ECLOUD04, 19/4/04 E.Benedetto, F.Zimmermann 21
Ongoing and Future plans
• Continue analytical approach to model electron cloud phenomena
• Comparison with HEADTAIL simulations.
• Produce instability diagrams for the electron cloud
• Investigations about
– what happens after the bunch had passed
– Longitudinal discontinuities in the electron plasma.