V.N. Litvinenko, 30 th FEL Conference, Gyeongju, Korea, August 28, 2008 PROGRESS WITH FEL-BASED...
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Transcript of V.N. Litvinenko, 30 th FEL Conference, Gyeongju, Korea, August 28, 2008 PROGRESS WITH FEL-BASED...
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
PROGRESS WITH FEL-BASED COHERENT ELECTRON COOLING
Vladimir N. Litvinenko, Ilan Ben Zvi, Michael Blaskiewicz, Yue Hao, Dmitry Kayran, Eduard Pozdeyev, Gang Wang
Brookhaven National Laboratory, Upton, NY 11973, USA
Oleg A. Shevchenko, Nikolay A. VinokurovBudker Institute of Nuclear Physics, Novosibirsk, Russia
George I. Bell, David L. Bruhwiler, Andrey SobolTech-X Corp., Boulder, CO 80303, USA
Yaroslav S. Derbenev, TJNAF, Newport News, VA, USA
Sven Reiche, UCLA, Los Angelis, CA, USA
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Content* What is Coherent electron Cooling? * Why it is needed?* Our plan of the comprehensive studies* Progress with Modulator, FEL, Kicker, PoP* Conclusions
Cooling intense high-energy hadron beams remains a major challenge for accelerator physics. Synchrotron radiation is too feeble, while efficiency of two other cooling methods falls rapidly either at high bunch intensities (i.e. stochastic cooling of protons) or at high energies (i.e. e-cooling). Possibility of coherent electron cooling based on high-gain FEL and ERL was presented at last FEL conference [1]. This scheme promises significant increases in luminosities of modern high-energy hadron and electron-hadron colliders, such as LHC and eRHIC. In this talk we present progress in development of this concept, results of analytical and numerical evaluation of the concept as well our prediction for LHC and RHIC. We also present layout for proof-of-principle experiment at RHIC using existing R&D ERL. In this paper we report on the progress in the development of the scheme of coherent electron cooling (CeC) since a specific scheme and its theoretical evaluation were proposed about an year ago [1].
[1] V.N. Litvinenko, Y.S. Derbenev, Proc. of FEL’07 Conference, Novosibirsk, Russia, August 27-31, 2007, p.268 http://accelconf.web.cern.ch/accelconf/f07
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Coherent Electron Cooling
Modulator
Kicker
Dispersion section ( for hadrons)
Electrons
Hadrons
l2l1 High gain FEL (for electrons)
Eh
E < Eh
E > Eh
Eh
E < Eh
E > Eh
Modulator Kicker
Electrons
Hadrons
l2
l1
High gain FEL (for electrons) / Dispersion section ( for hadrons)
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Decrements for hadron beamswith coherent electron cooling
Machine SpeciesEnergy GeV/n
Trad.StochasticCooling,
hrs
Synchrotron radiation, hrs
Trad.Electron cooling
hrs
CoherentElectron
Cooling, hrs 1D/3D
RHIC PoP
Au 40 - - - 0.02/0.06
eRHIC Au 130 ~1 20,961 ~ 1 0.015/0.05
eRHIC p 325 ~100 40,246 > 30 0.1/0.3
LHC p 7,000 ~ 1,000 13/26 0.3/<1
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Comprehensive studies Analytical, Numerical and Computer Tools to:1. find reaction (distortion of the distribution function of
electrons) on a presence of moving hadron inside an electron beam
2a. Find how an arbitrary f is amplified in high-gain FEL
2b. Design cost effective lattice for hadrons + coupling3. Find how the amplified reaction of the e-beam acts on the hadron (including coupling to transverse motion)
fe
t fe
v eE m fe
r v 0;
r h (t)
r o
v ht;
E 4ene
Zne
r r h (t) fed
v 3
.
f fo f
fexit (r ,p ,t) fo exit (
r ,p ) K
r ,p ,r 1,p 1,t t1 f (
r 1,p 1, t1)d
r 1 dp 1dt1
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Modulator Dimensionless equations of motion
f e
t f e
v eE
m f e
r v 0;
r h (t)
r o
v h t;
E 4ene
Z
ne
r r h (t) fed
v 3
.
R v
vz
; Tvhx
vz
; Lvhz
vz
; Z
4neR2s3
;
Aa
s; X
xho
a;Y
yho
a.
t /p; v =vz
; r
vz/p; p
2 4e2ne
m
Parameters of the problem
fe
fe
g fe
0;
g
eE
mp2s
;
n
g Z
s3ne
i(t) fed3 ;
n .
s rDzvz
/p
+Ze
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Perturbation caused by a hadron (co-moving frame)Analytical: for Lorentzian electron plasma, G. Wang and M. Blaskiewicz, Phys Rev E 78, 026413 (2008)
Numerical (VORPAL @ TechX)
Ion at rest
vhz 10 vz
˜ n r ,t Znop
3
2vxvyvz
sin 2 x - vhx /p
rDx
2
y - vhy /p
rDy
2
z - vhz /p
rDz
2
2
0
pt
d
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
QuickTime™ and aYUV420 codec decompressor
are needed to see this picture.
VORPAL @ TechX
QuickTime™ and aYUV420 codec decompressor
are needed to see this picture.
QuickTime™ and aYUV420 codec decompressor
are needed to see this picture.
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Modulator KickerDispersion section ( for hadrons)
Electrons
Hadrons
l2
l1 High gain FEL (for electrons)
Eh
E < Eh
E > Eh
Eh
E < Eh
E > Eh
CeC: FEL response
f input(r ,p ,t) fo input(
r ,p )f (
r ,p ,t)
fexit (r ,p ,t) fo exit (
r ,p ) K
r ,p ,r 1,p 1, t t1 f (
r 1,p 1, t1)d
r 1 dp 1dt1
1D FEL response
exit (t;z) = o G ;z (t ;0)d
G ;z Re ˜ G z e io
0 2c
o
;
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
FEL’s Green Function 1D - analytical approach3D - 3D FEL codes RON and Genesis 1.3
FEL parameters for Genesis 1.3 and RON simulations
FEL gain length: 1 m (power), 2m (amplitude)
Main FEL parameters for eRHIC with 250 GeV protons
Energy, MeV 136.2 266.45
Peak current, A 100 o, nm 700
Bunchlength, psec 50 w, cm 5
Emittance, norm 5 mm mrad aw 0.994
Energy spread 0.03% Wiggler Helical0
0.2
0.4
0.6
0.8
1
0 50 100 150 200 250 300 350 400
RON
Genesis
0
0.2
0.4
0.6
0.8
1
Mod
ulat
ion,
nor
mal
ized
Slice number, in unit of 0
Modulation after 20m of FEL
G ;z Re ˜ G z e io
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Response - 1D FEL
E.L.Saldin, E.A.Schneidmiller, M.V.Yurkov, The Physics of Free Electron Lasers, Springer, 1999
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Response - 1D FEL after 10 gain lengths
-500
0
500
1000
1500
2000
2500
3000
3500
-2 0 2 4 6 8 10 12
Re ImAmplitude
Gre
en F
unct
ion
In units of slippage per gain lenght
Green-functionenvelope (Abs, Re and Im)
Maximum located at 3.744 slippage units,(i.e. just a bit further that expected 3 and 1/3)
The Green function (with oscillations) had effective RMS length of 1.48 slippage units.
vg c 2 vz
3c 1
1 aw2
3o2
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Genesis: 3D FEL
Evolution of the maximum bunching in the e-beam and the FEL power simulated by Genesis. The location of the maxima, both for the optical power and the bunching progresses with a lower speed compared with prediction by 1D theory, i.e. electrons carry ~75% for the “information”
Evolution of the maxima locations in the e-beam bunching and the FEL power simulated by Genesis.Gain length for the optical power is 1 m (20 periods) and for the amplitude/modulation is 2m (40 periods)
vg c 3 vz
4c 1
3
8
1 aw2
o2
©Y.Hao, V.Litvinenko
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
3D FEL, RON codeRHIC 250 GeV, FEL @ 0.7 m,
gain length - 40 periods (amplitude). 20 (power)
©O.Shevchenko
20 GL
18 GL
16 GL
-300
-200
-100
0
100
200
300
400
500
-100 0 100 200 300 400
Data J10c4Re(
mod)
Im(mod
)
E
mod
, a.u
.
Slice
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Genesis: 3D FEL
Evolution of the normalized bunching envelope
The Green function (with oscillations) after 10 gain-lengths had also smaller effective RMS length [1] of 0.96 slippage units (i.e. about 38 optical wavelengths, or 27 microns
0
0.2
0.4
0.6
0.8
1
0 50 100 150 200 250 300
bunch_norm
Value, 0mValue, 2mValue, 4mValue, 6mValue, 8mValue, 10mValue, 12mValue, 14mValue, 16mValue, 18mValue, 20mValue, 22mValue, 24m
m
ax
Slippage, in units of 0
©Y.Hao, V.Litvinenko, S.Reiche
10-8
10-7
10-6
10-5
0.0001
0.001
0.01
0.1
1
0 100 200 300 400 500
Bunching, normalized amplitudeValue, 0mValue, 2mValue, 4mValue, 6mValue, 8mValue, 10mValue, 12mValue, 14mValue, 16mValue, 18mValue, 20mValue, 22mValue, 24m
Slippage, in units of 0
0.0001
0.01
1
100
104
106
0 100 200 300 400 500
Optical powerValue, 0mValue, 2mValue, 4mValue, 6mValue, 8mValue, 10mValue, 12mValue, 14mValue, 16mValue, 18mValue, 20mValue, 22mValue, 24mP
ower
Slippage, in units of 0
Evolution of the bunching and optical power envelopes(vertical scale is logarithmic)
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Kicker: output from Genesis propagated for 25 m
0m 5m 10m
25m
©I.Ben Zvi0
0.1
0.2
0.3
0.4
0.5
0.6
0 5 10 15 20 25
Bunching in the Kicker, 700 nm
Bunching
Bu
nch
ing
Distance, m
QuickTime™ and aTIFF (LZW) decompressor
are needed to see this picture.
15m
QuickTime™ and aTIFF (LZW) decompressor
are needed to see this picture.
20m
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
IR-2 layout for Coherent Electron Cooling proof-of-principle experiment
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Conclusions• These initial studies did not find any phenomena,
which challenges the concept of CeC• Our initial CeC estimations passed the test• At the same time, we found a number of new and
interesting details to pursue further• Future studies will refine the model and improve the
quality of predictions• We plan to test validity of the concept
experimentally in Proof-of-Principle experiment using BNL’s R&D ERL installed in one of available IPs at RHIC
• Supported by office on Nuclear Physics, US DoE
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
V.N. Litvinenko, 30th FEL Conference, Gyeongju, Korea, August 28, 2008
Response - 1D FEL; z=13mEffect of energy spread and space chargeRed - amplitude, Blue - phase
@
©G.Wang