Yuelin Li and Stephen V. Milton Advanced Photon Source, Argonne National Laboratory
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Transcript of Yuelin Li and Stephen V. Milton Advanced Photon Source, Argonne National Laboratory
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Intensity and pulse shape effect on the Intensity and pulse shape effect on the spectral and angular distribution of spectral and angular distribution of
nonlinear Thomson scattering*nonlinear Thomson scattering*
Yuelin Li and Stephen V. Milton
Advanced Photon Source, Argonne National Laboratory
Argonne, IL 60565
*Supported by the U. S. Department of Energy, Office of Basic Energy Sciences
Contract No. W-31-109-ENG-38
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Electron dynamics and radiation in high intensity laser fieldsPonderomotive scatteringViolent accelerationHarmonic and broadband radiation….
Laser acceleration of electronsMeV and GeV electron acceleration…..
Ultrafast X-ray radiation generationNonliear Thomson scattering into X-rayBremsstrahlung X-ray ….
Background and relatedBackground and related
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
GeometryGeometry
Y.I. Salamin et al
Only electrons initially at rest and on axis are considered, x0=0, 0=0, =0.8 m, w0=10 m, Zr=400 m.
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
FormulaFormulaField: angular spectrum representation
,4
,24
,4
420
23030
20
32
2
230
22
120
Ir
xEE
IrIkrk
xyEE
Ir
yI
rk
yxI
EE
z
y
x
420
32
2
230
22
120
4
,4
,
Ir
y
c
EB
Ir
xI
rk
xyI
c
EB
c
EB
z
y
yx
,)()cos()
1
11(
,)(1
)sin(
,)(1
)sin(
,)()sin()11(
2012
1
0
4/4
3002
1
0
4/3
2012
1
0
4/2
0021
0
4/1
22
22
22
22
dbbrbkJb
eI
dbbrbkJb
eI
dbbrbkJb
eI
dbbrbkJbeI
bb
bb
bb
bb
.
,1
,1
22
00
200
yxr
wk
bzktb
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
FormulaFormula
Energy spectrum calculation by Lienard-Wiechert potentials
).(,,0
0
0
Bm
pEepdtpppdt
pr
The dynamics is solved numerically
.)(4
2)/(
2
222
dtennc
e
dd
Id crnti
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Single electron caseSingle electron caseMomentum and spectra
0 10 20 30 40 50
0.0
0.5
1.0
0.0
0.5
1.0
0.0
0.5
1.0
a0=0.01, =/2
h (eV)
a0=1, =1.
a0=3, =0.5
d2 I/d
dE
(a.
u. )
-1
0
1
-20 0 20 40 60
-0.01
0.00
0.01
-3
0
3
6
a0=1
px,
pz/m
c
a0=0.01
Time (fs)
pz a
0=3
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Single electron trajectory, R-Single electron trajectory, R-frameframe
-0.075 -0.050 -0.025 0.000 0.025 0.050 0.075-0.625
-0.500
-0.375
-0.250
-0.125
0.000
0.125
0.250
0.375
0.500
x/ 0
z/0
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Single electron: Spectrum Single electron: Spectrum details details
1 2 3 4 5
0
1
2
3
4
5
e
d
c
b
a
dE
/dd
(a
.u.)
h (eV)Fig. 1. Spectra of single electron irradiated by (a)-(d) 20-fs laser pulse with a0=3 for =40 at
=0, 30, 60, and 90, and (e) with quasi-flat-top 80-fs pulse with a0=3 for =40 at = 90.
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Single electron: Angular Single electron: Angular distribution distribution
0
30
6090
120
150
180 0
30
6090
120
150
180
0
30
6090
120
150
180 0
30
6090
120
150
180
0
30
6090
120
150
180 0
30
6090
120
150
180
(b)
(c) (d)
(e) (f)
(a)
Fig. 2. Radiation pattern of the second (solid) and third (dashed) harmonics at =90 (left panels) and 60 (right panels) for (a)-(b) 80-fs quasi-flat-top pulse a0=3, (c)-(d) 20-fs pulse with a0=3 and (e-f) 20-fs pulse with a0=2.
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Single electron: conclusion Single electron: conclusion
1 2 3 4 5
0
1
2
3
4
5
e
d
c
b
a
dE
/dd
(a
.u.)
h (eV)
Observations
1. Red shift with intensity and polar angle, explained by theory
)cos1()2/(1 20
a
nn
2. Spectral broadening, modulation, and over lapping are pulse- shape and intensity- dependent and not discussed previously.
3. Angular distribution is also intensity-and pulse shape-dependent
0
30
6090
120
150
180 0
30
6090
120
150
180
0
30
6090
120
150
180 0
30
6090
120
150
180
0
30
6090
120
150
180 0
30
6090
120
150
180
(b)
(c) (d)
(e) (f)
(a)
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Collective effects Collective effects
For a collection of electrons, the radiation is calculated as
.)(4
2
)/(
2
222
dtennc
e
dd
Id
j
crntij
jj
.)(4
2)/(
2
222
j
crntij dtenn
c
e
dd
Idjj
When the positions of the electrons are totally random, the only terms survive the integration are the individual terms of each electrons, hence the radiation for a collection of electrons can be approximated as
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Z-dependence: Spectra Z-dependence: Spectra
0 1 2 3 4 5 h (eV)
4ZR
3ZR
2ZR
ZR
0
-ZR
-2ZR
-3ZR
h0=1.55 eV
w0=10 m
zr=400 m
a0=3
=90°=42°
-4ZR
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Target thickness dependence Target thickness dependence
0 1 2 3 4 5
h (eV)
3ZR
5ZR
7ZR
h0=1.55 eV
w0=10 m
zr=400 m
a0=3
=90°=42°
9ZR
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Target thickness: angular Target thickness: angular distribution distribution
0.00
0.25
0.50
0.75
1.00
0
30
60
90
120
150
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210
240270
300
330
0.00
0.25
0.50
0.75
1.00
0.00
0.25
0.50
0.75
1.00
0
30
60
90
120
150
180
210
240270
300
330
0.00
0.25
0.50
0.75
1.00
0.00
0.25
0.50
0.75
1.00
0
30
60
90
120
150
180
210
240270
300
330
0.00
0.25
0.50
0.75
1.00
0.00
0.25
0.50
0.75
1.00
0
30
60
90
120
150
180
210
240270
300
330
0.00
0.25
0.50
0.75
1.00
3zr
2nd 3rd
5zr
7zr 9z
r
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
Conclusion Conclusion
Nonlinear Thomson scattering emission spectra and angular distribution are sensitive to the laser intensity, pulse shape and target configuration both on the microscopic and macroscopic level, showing spectral shift, broadening and mixing between harmonics.
2002 CLEO, Long Beach, California, May 19-24, 2002, Session CWA
References References
1. E. S. Sarachik and G.T. Schappert, “Classical theory of the scattering of intense laser radiation by free electrons,” Phys. Rev. D 1, 2738-2753 (1970).
2. S. K. Ride, E. Esarey, and M. Baine, “Nonlinear Thomson scattering of intense laser pulses from beams and plasmas,” Phys. Rev. E 48, 3003-3021 (1993).
3. S-Y Chen, A. Maksimchuk, and D. Umstadter, “Experimental observation of relativistic nonlinear Thomson scattering,” Nature 396, 653-655 (1998).
4. K. Ta Phus et al., “Synchrotron-like radiation produced from an intense femtosecond laser system,” OSA Conference on Applications of High Field and Short Wavelength Sources IX, October 21–24, 2001, Palm Springs, California.
5. B. Quesnel and P. Mora, “Theory and simulation of the interaction of ultraintense laser pulses with electrons in vacuum,” Phys. Rev. E 58, 3719-3732 (1998), and references therein.
6. J. D. Jackson, Classical Electrodynamics (Wiley, New York, 1976).7. Y. Ueshima, Y. Kishimoto, A. Sasaki and T. Tajima, “Laser Larmor X-ray radiation
from low-Z matter,” Laser Part. Beams 17, 45-58 (1999).