photoinjectors & beam manipulations for lcs and fels & collimation [mccpb, chapters 5,6]...
TRANSCRIPT
Photoinjectors & Beam Manipulations for LCs and FELs & Collimation
[MCCPB, Chapters 5,6]
• manipulations in photoinjectors– space-charge compensation– flat beam generation
• emittance exchange• some other beam manipulations for FELs• collimation in linacs & storage rings
sources of electron beams
requirements: small emittance high charge, high repetition rate, possibly high degree of polarization
• thermionic guns• dc guns with laser photocathodes• photo-cathode rf guns
(SLC)
rf wave
laser beam
e-
cross section of an earlyBNL S-band rf gun(J. Clendenin, 1996)
most popular in modern e- accelerators (in particular, if low emittances aredesired); high-power pulsed laser illuminates photocathode placed on the end wall ofan accelerating cavity, electrons are immediately accelerated in rf field
normalized emittance determined by three effects:• thermal emittance – initial transverse momenta• rf emittancee – from time-dependent focusing force• space-charge force
techniques for shaping and preserving the beam emittance from such injector:
space-charge compensation using solenoidsgeneration of a flat-beam transverse-longitudinal emittance exchange
rf photo-injector
z
r
a
zeNE br 2
02
r
ac
zeNvB b
2202
r
eEevBeEF rr 2
1
space-charge force
longitudinal bunch profile
assume transverse uniformdistribution with radius a
transverse view
if (z) not constant, different longitudinal slices will experience differentfocusing force Fr
x
x’ different slicesrotate at differentspeedprojected emittanceis increased
space-charge compensation
radius a
after drift of length s: Gcm
sNe bxN 2
00
2
16
6.02.0 G depends on shape of distribution
2,2
1,,
),(,,'
sasr
ssr
)(2
2
fd
d
zz
zf
)(
)(2
),(
),('
ldd
dl
zzz
zz
r
r
f
azzza ddl
Nyx
2222
, )(22
1
place lens of focal length f after distance zl
after total distancezd+zl:
emittance is indeed 0 at chosen value of f
in reality not constantbut above scheme reduced the emittance by a factor 10 in Los Alamos studies
‘space-chargecompensation”(B. Carlsten, ~1993)
bunch slices arerealigned
assume constant
rf
r1
'
normalized longitudinalcoordinate
normalized transverse coordinate
a
after first drift after solenoid
after finaldrift
all particlesare on one line!
center
edge
beware of bifurcation!
r
r’ r’
r
strong space charge
weak space chargebunch center
bunch edgephase-spacebifurcation
important design criterion for photo-injectors: minimize fraction of beam crossing over!
“crossover”
similar techniques to correct correlated growth in projected emittance due to nonlinear forcecan be applied elsewhere
flat-beam transformation
• proposed by Y. Derbenev to convert round
beam into flat or vice versa (1998)
• in particular can produce a flat beam from a
photoinjector if source is placed in solenoid field
and afterwards passed through a (skew) FODO
channel with /2 different phase advance in x & y
zy
zx
By
BdsB
Bx
Bx
BdsB
By
2
11'
2
11'
0
0
0
0
0
0
0'
'
kx
y
ky
x
y
y
x
x
kick at exit of solenoid
phase-space vector at exit of solenoid
quadrupole channel withphase advance difference /2 in x and y choose=1/k
this is a flat beamtilted by 45 degree!
if we use skew-quad.channel, could geta flat beam in x
0
0
0
0
0
0
0
0
10100
000
0010
0001
'
'
kx
y
ky
x
kx
y
ky
x
y
y
x
x
however initial beam has also some rms slope (temperature)
20
202
1,
1,
20
1,
'41
'
2
1
x
x
y
x
yy
k
k
0'0'00 , yxyx assuming
product of x and y emittances approximately conserved
experimental tests at Fermilab A0 line demonstrated the feasibilityof this scheme
simulated evolution of transverse emittances along the FNPL beamline for standard nominal settings
FNAL Flat Beam Experiment
schematic layout
Y.-E. Sun
Simulated and measured beam transverse density evolution. The consecutive plots corresponds to location X3, X4, X5, X6, X7 and X8. Dimensions are in mm.
Overview of the RFTB section. The letters N, S and X represents normal and skew quadrupoles, and diagnostic stations. Dimension are in mm.
simulatedmeasured
FNAL Flat Beam Experiment – cont’d
Y.-E. Sun
general emittance exchange between two planes
with2 magnitude of the coupling and is the sum of the squares of the four elements of the normalized coupling block of the transfer matrix, i.e. U :
where
and
M. Cornacchia and P. Emma
which can be rewrittenas
equal initial uncoupled emittances will always remain equal through a symplectic map; similarly, equal uncoupled emittances cannot be generated from unequal uncoupled initial emittances - setting |A| = 1/2 produces equal emittances, but they are then highly coupled with 𝜆2≠0
transverse to longitudinal emittance exchange- EEX
• proposed by M. Cornacchia and P. Emma to reduced the transverse emittance (and also shrink the bunch length) for FELs (2002)
• realized by placing a transverse deflecting mode radio-frequency cavity (“crab cavity”) in a magnetic chicane
Initial (top) and final (bottom) phase space tracking plots. The horizontal and longitudinal emittances are completely exchanged, as predicted.
M. Cornacchia and P. Emma
transverse to longitudinal emittance exchange – experimental EEX demonstration at FNAL A0 line
T. Koeth, 2009Layout of the A0 Photoinjector with straight ahead and EEX beamline sections.
EEX - key ingredients1. half chicane (dipole magnets) creates correlations between x and
2. deflecting cavity changes energy of particles with transverse offset x and and deflects particles horizontally depending on the longitudinal position
3. another half chicane thin lens deflecting cavity
P. Emma and M. Cornacchia
The 4x4 (horizontal-longitudinal) emittance exchange matrix as a function of TM110 cavity strength. The cavity is off at k=0% and is energized to the ideal emittance exchange strength at k=100%. The circles are measured points, the green (lighter) lines are fits to the data, and the red (darker) lines are calculated values. T. Koeth, 2009
calculated matrix elements
the 4x4 (horizontal-longitudinal) measured matrix
T. Koeth, 2009
nonzero due to finite cavity length
Relative output 1/σp·σz product map against input quadrupole currents. The white cross hairs indicate a choice for EEX operation.
Calculated ratio of εx,in/(σp·σz)out over input quad scan. The white and green cross hairs indicate the operating points for Feb 6 and Feb 11 data sets respectively.
T. Koeth
Transverse input parameters were tuned (by adjusting input quadrupoles) for a minimum output bunch-length energy-spread product.
February 11, 2009, Direct EEX Data Set, Reflecting Input and Output rms Normalized Emittances
T. Koeth, 2009
Undulator RadiationP. Schmüser
Undulators & Free Electron Lasers
Z. Huang,P. Schmuser
undulator
undulator parameter
fundamental wavelength of undulator radiationin forward direction
condition for sustained energy transfer from electron to light wave
exponential growth and saturation of the FEL power in SLAC LCLSat =0.15 nm; initiated by Self Amplified Spontaneous Emission (SASE) process
P. Emma,PAC09
linac based X-ray FEL - LCLS
1-D power gain length
e- density
Pierce parameters
saturation power
typical requirements
Z. Huang,P. Schmuser
combination flat-beam gun & EEX
standard rf photocathode gun:x,y
gun~ 1 m, zgun ~ 0.1 m
flat beam scheme:x,, y z) → (10, 0.1, 0.1) m
followed by transverse-to-longitudinal exchange:x,, y z) → (0.1, 0.1, 10) m
with much improved FEL performance(3x shorter undulator)
P. Emma et al, 2006
=0.4 Å
FEL power as a function of z/Lg0 (1D power gain length) in a seeded FEL and a SASE FEL (soft X-ray FEL FLASH)
P. Schmuseret al.
SASE and seeded FEL - FLASH
FEL seedingSASE exhibits shot-to-shot fluctuations in wavelength and limitedcoherence length (many uncorrelated spikes along the bunch length)
various seeding methods proposed to improve coherencelength of SASE radiation:•High harmonic generation (HHG) in gas; VUV•Self seeding: SASE signal produced by short undulator passed
through monochromator and serves as seed radiationfor main undulator
•High-gain harmonic generation (HGHG) electron is energy-modulated by interaction in an undulator by interaction with powerful laser;magnetic chicane converts energy modulation into density modulation; then second undulator for coherent emission fromdensity modulated beam at higher harmonic frequency
•Echo enabled harmonic generation (EEHG): second modulator followedby second chicane; electron beam interacts twice with two laserpulses in two modulators; density modulation at a very highharmonic number
HGHG FEL scheme
R56
laser
modulator radiator
phase space distribution
D. XiangG. Stupakov
e- shiftby /4
EEHG FEL scheme
R56(1)
laser 1
modulator 1 radiator
laser 2
Modulator 2
R56(2)
phase space distribution
e- shiftby >10
currentdistribution
D. XiangG. Stupakov
A.A. Zholends,M.S. Zolotorev,PRL 76, 6 (1996)
what happens in a modulator?laser
laser radiation spontaneous undulator radiation
total electric field
total field energy
: relative phase of the laser light wave and electron wiggling trajectory in undulator
spontaneous radiation of electrons in an undulator
→ amplitude of e- energy modulation after the modulator
applications of modulators:-laser heating (suppression of microbunching
instability in bunch compressors), e.g. for FELs-FEL HGHG -FEL EEHG-femtosecond pulse generation (bunch “slicing”)
in storage rings…
A.A. Zholends,M.S. Zolotorev,PRL 76, 6 (1996)
an alternative formula can be found inZ. Huang et al. PRST-AB 7, 074401 (2004)
femtosecond pulse generation at the ALSR.W. Schoenlein et al, SCIENCE, Vol. 287 March 2000
Laser interaction with electron bunch in a resonantly tuned wiggler.
Transverse separation of modulated electrons in dispersive bend of the storage ring
Separation of femtosecond synchrotron radiation at the beamline image plane.
E=1.5 GeV, E=1.2 MeVMu=19 periods, u=16 cm,K=13, L=100 fs, AL=400 J, L=800 nm
electron bunch distribution (as a function of horizontal displacement x and time) at the radiating bend magnet, following inter-action with the laser pulse in the wiggler, and propagation through 1.5 arc sectors of the storage ring
collimation• removal of beam halo, which otherwise causes
background in the detector (el.-magnetic showers or muon production when lost near detector; or synchrotron radiation when passing at large amplitudes) or, for s.c. proton rings, could quench the magnets
• controlled removal (activation of only one area)
• multistage systems frequently employed
• collimators also serve to protect the rest of the accelerator against catastrophic beam losses due to failure (machine protection)
• collimator survival collimator impedance
challenge for many future projects
example: collimator at the SNS high-energy beam-transfer line
beam usually not of ideal shape• beam-gas Coulomb scattering
• beam-gas bremsstrahlung
• Compton scattering off thermal photons
• linac wake fields
• halo from the source or from damping rings
• halo from ring-to-linac transport and bunch compression,…
collimation in linear colliders
Yes, measured beam distribution at the end of the SLAC linac (projection on the x-y plane)!
Is there halo in linear colliders?
let us look at the SLC prediction…
DispersionSpace charge (?) Elastic scattering off residual gasResidual-gas bremsstrahlungTouschek scatteringIntrabeam scatteringDark currentsNonlinear magnetic fields Scattering off thermal photonsScattering off laser fieldIncoherent & nonl. wake fieldsSynchrotron radiation (coherent & incoherent)Ion or electron-cloud effects
More Complete List of Candidate Processes
close to the source, in bendseverywhere
everywhereeverywhere
everywhere
scatteringphoto gun
cavities, linacring, linac
e.g. collimatorsin bends
e- or e+ beams
linac
at the SLC
• muons, SR, showers were all problems
• more and more collimators were added over the years upstream of the final focus
• magnetized toroids were placed between collimators and collision points to reduce the number of muons reaching the detector
• it was difficult to model the halo
schematic of a collimation system for future linearcolliders consisting of spoiler and absorber pairs
scattering off thin spoiler increases beam size on subsequent absorber to prevent damage
collimation is done for different betatron phases and in energy
collimation in storage rings
• beam-gas Coulomb scattering
• beam-gas bremsstrahlung
• Compton scattering off thermal photons
• nonlinear fields (resonances, tune drifts,…)
• space charge
• intrabeam scattering, Touschek effect
• beam-beam interaction
halo generating processes
measurement of beam tailsin LEP-2 (80-100 GeV)using movable collimators
result of Monte-Carlo simulation
beam-gas scattering and thermal-photon scattering
(Courtesy H.. Burkhardt, 1998)
cN
N halo generation rate
density ofresidual gasor of thermalphotons
halo generation by scattering processes
cross section
total cross sectiondepends on limits for ,
Bremsstrahlungelectrons lose energy in inelastic scattering events with theresidual gas (e.g., SLAC-PUB-8012 and references therein)
3/1
22
0
2
0
183ln4
1
where
3
4
3
41
ZA
ZNr
X
kkkXN
A
dk
d
Ae
A
brems
total cross section for energy loss > 1% is 6.5 barn for CO
bB
bremsb
ebrems
LNTk
pN
ZZr
183
lnln3
163/1min
22
remains importantat high energies
k: energy of photon radiatedin bremsstrahlung event
Elastic Coulomb scattering
total cross section
23/82.0 Cel Z
for scattering above minimum angle
3/1min 4.1 where, Za
pae
bB
elb LNTk
pN
scattered electrons:
scattering angle decreases at higher energies
at large amplitudes tail from elastic gas scattering like ~1/y3
TorRauben-heimer,1992
damping ring
Scattering off thermal photonstotal cross section is close to the Thomson cross section=8/(3r0
2)=0.665 barn
density of photons is =2x107 T3/m3; at room temperature =5.3x1014/m3
number of scattered particles: Nb= L Nb
maximum energy loss ymax=x/(1+x), wherex=15.3 [E/TeV] [E/eV] cos2 (/2)
average photon energy E=2.7 kBT (10 meV at 300 K)
this process becomes relevant for beam energies above50 GeV, when the mean relative energy loss in a scatteringevent exceeds 1%
number of photons per radian:
Synchrotron radiation
GeV rad
120
32
5
d
dN
critical energy: ccc EEEc
E ,,
3
, 32.0315
8 and
2
3
energy spread:
2
52
324
55eerms r
emittance growth:5211
35 GeVm102 where Qb
xQx Cl
HEC
tails:2
4
,
/
2, 2
where/28
39 ,
EcCP
EE
e
E
P
dE
dN
c
EE
c
c
at both SLC and LEP the synchrotron radiation was minimized by weakening the last bending magnet closest to the interactionpoint by factor ~10, which reduced the critical energy as well as the number of photons emitted per unit length
in addition radiation masks were installed to absorb photons emittedin the weak bend and in upstream bends
layout of the straight sectionaround IP4 or IP8 in LEP;COLH, COLV, COLZ are masks(Courtesy H.. Burkhardt, 1998)
residual background in LEP arose mainly from multiply scattered photons;reflectivity of soft X-rays is close to 100% for impact below critical angle~30 mrad keV/Ereduced by coating or surface roughening
LEP masks provided complete shielding against direct photons andagainst singly scattered photons:
(Courtesy H.. Burkhardt, 1998)
H. Burkhardt
synchrotron-radiation shields for FCC-ee?
Summary
photo-injectors, space-charge compensation
generation of a flat beamgeneral emittance exchangetransverse-longitudinal emittance exchange
FEL laser seeding and bunch slicing
halo generationcollimation in linear colliders & storage rings