Kansas State University
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Transcript of Kansas State University
Kansas State University
High energy 6.2 fs pulses
J. R. Macdonald Laboratory
Shambhu Ghimire, Bing Shan, and Zenghu Chang
Kansas Light Source Group
Summary
• A shorter pulse ?• A higher energy pulse?• Limitations for producing such pulses• Our approach of obtaining a higher
energy• Measurement of the pulse• Further possibilities
Applications of attosecond pulses
Time scale
as psfszs10-18 s 10-15 s 10-12 s10-21 s
Progress
HHG
e-
Attosecond pulse train by HHG
Half Cycle
HHG as pulse Train
Driving fs Pulse
Gastunnel
ionization+ re-collision
e-
E(t)
Experimental ObservationHHG Spectrum: Discrete Spectral
Lines
Discrete harmonic orders in the plateau
-Spatial analogy of pulse train interference
Single slit
Double slit
Multi slit
Diffraction patterns(spatial frequency)
Discrete pattern at plateau analogy to multi-slit diffraction
Shorter fs-pulse to get a single atto-pulse
Harmonic generation
??
Super continuum at near cutoff
With ~25 fs pulses
With ~10 fs pulses
With ~5 fs pulses
fs-pulses Atto-pulses
??
Traditional method : generation of single atto-second pulses
P. B. Corkum, N. H. Burnett, and M. Y. Ivanov, Opt. Lett. 19, 1870 (1994)V. T. Platonenko and V. V. Strelkov J. Opt. Soc. Am. B 16, 435 (1999)
p
Left Circular Pulse
Right Circular Pulse
Td
e-
e-
e-
Polarization gating for a single atto-pulse
Ellipticity dependent pulse
1) Polarization gating method
Shorter gate
Using a shorter pulse
Using a longer delay
High energy, ultra-short pulse
d
p
Tt
2
2.0 3.0
available short pulse
2) Traditional method
To cover broader wavelength range of a atto-pulse
Limits
final energy at gate
Our goal
To scale up the energy of a few cycle pulses
I t( ) Io e
4 ln 2( )t
2
n I( ) n0
n2I t( ) t
2 n
2 I t( ) L
o
o
Spectral broadening by SPM
I (t)
n(t)
no
wtd
d
t
o
t( )
t( )
Non linear medium
I (w)
I (w)
Pulse compression by - GVD
Self Phase modulation
Compressor
Experimental setupGeneration of a few cycle pulses
FROG
f = 1mO D = 6mmI D = 0.4mm
f = 2.5 mAr- gas
Hollow core fiber/ chirp compressor technique
Previous work and Limitations
• Self focusing along with self phase modulation• Self de-focusing by plasma formation
Higher Energy ~ 0.5 mJ1
Shorter Pulse Duration ~ 5 fs 1
• Achievable spectral broadening by SPM • Bandwidth limitation of compressor technique
1S. Sartania, Z. Cheng, M. Lenzner, G. Tempea, Ch. Spielmann, and F. Krausz, Optic Letters, 22,20 (1997).
Limitations
I (r)
I (r)
no+n2I (r)
no - n e
Self-focusing
Self-defocusing
f=1m
f=1m
n (I) = no + n2 I
n (I) = no - Ne/ 2Ncr
Our approach
Higher Energy
Shorter Pulse Duration
• Broader spectrum with higher input circular polarization
Linear polarization input Circular polarization input
• lower self-focusing with circular polarization• Reduced ionization greatly reduces self de-
focusing
Reducing self focusing
n (r) = no + nL2 I (r)
n (r) = no + nC2 I (r)
Radial distance in micrometer
0
2 1013
4 1013
6 1013
6 1013
0
I r( )
300300 r
190 80 0 140 2500
1 10 6
2 10 6
3 10 6
4 10 6
5 10 6
4.704 106
1.378 107
nL r( )
nC r( )
250250 r
A Gaussian pulse
Nonlinear index of refraction
nC2
nL2= 1.5
Preserving self phase modulation
b4 a n
2 I L 0
F f 1b
a
2
n (r) = no + nL2 . I (r) n (r) = no + nC2
. I (r)
Chirp parameter Output band width
Linear polarization input Circular polarization input
=
Reducing self defocusing
F
2 Fo
F.A. Ilkov et al. J. Phys. B, 25 (1992)A.M. Perelomov et al. JETP, 24, (1966)
Selection rule : Less ionization channels in circular
Reducing field by 0.7 reduces ionization by >1 order
Multiphoton ionization Tunneling ionization
Reducing self defocusing
)()( 0 InnIn cr
gas
N
NIIPIn
.2
).()(
Lower field of circular input lead to decrease in ionization
By using circular polarization input
nC F( ) 0.0086IPC F( )nL F( ) 0.0086IPL F( ) IPL
Combined effects : SF and SDF
0)( nRrn
SDFSF
60 107.4)0( nrn 008.0)0( 0 nrn
0)( nRrn 0)( nRrn
Linear input
Circular input
0)0( nrn
0)( nRrn
0)0( nrn
Complicated profile
Single mode
Measured spatial profiles
a) b) c) d)
Input Energy
0.55 mJ 1.0 mJ 1.2 mJ1.2 mJ
vacuum Ar-gas Ar-gas Ar-gas
Linear
Circular
Throughput energy in vacuum
0.4 0.6 0.8 1.0 1.20.3
0.4
0.5
0.6
0.7
0.8
0.9
Outp
ut E
nerg
y (
mJ)
Input Energy (mJ)
Linear Circular
Scaling up energy by circular polarization
Ar-gas pressure at ~ 1 atm
0.6 0.8 1.0 1.20.35
0.40
0.45
0.50
0.55
0.60
0.65
Linear-Threshold
Circular-Threshold
Outp
ut E
nerg
y (
mJ)
Input Energy (mJ)
Circular Linear
Scaling up energy by circular polarization
0.6 0.8 1.0 1.2 1.4
0.4
0.5
0.6
0.7
0.8
Linear-Threshold
Circular-Threshold
Outp
ut E
nerg
y (
mJ)
Input Energy (mJ)
Linear Circular
Ar-gas pressure at ~ 0.5 atm
Broader spectrum for circular input
Ar-gas pressure at ~ 0.5 atm
600 700 800 9000.0
0.5
1.0
Inte
nsi
ty (
norm
aliz
ed)
Wavelength (nm)
At circularthreshold
At linearthreshold
CircularAt linearthreshold
Time Delay Stage
Spectrometer and CCD
BBO Crystal
I(t)
lens
50% BS
I (t-ז)
Tim
e (f
s)
Wavelength (nm)
Filter
Measurement of the pulses
FROG- Experimental setup
Measurement of pulsesmeasured FROG traces
Input pulse Output pulse
Wavelength (nm) Wavelength (nm)
Tim
e d
ela
y (
fs
) Tim
e d
elay
( fs )
1 pixel horizontal = 0.291 nm, 1pixel vertical = 0.716 fs
Measurement of input pulses
-100 -50 0 50 1000.0
0.5
1.0
33 fs
Intensity Phase
Time (fs)
Inte
nsity (
norm
aliz
ed)
0
5
10
15
20
Phase (ra
d)
Measurement of input pulses
725 750 775 800 825 850 8750.0
0.5
1.0
Reconstructed measured
Wavelength (nm)
Inte
nsity
(no
rmal
ized
)
Time
Time
(d)
Fre
que
ncy
Fre
que
ncy
Measured
Reconstructed
Measurement of output pulses
-20 -10 0 10 200.0
0.5
1.0
6.2 fs
Intensity Phase
Time (fs)
Inte
nsity (
norm
aliz
ed)
0
2
4
6
8
10
Phase (ra
d)
0.6 mJ, 6.2 fs pulses at rep. rate of 1k Hz
Measurement of output pulses
600 700 800 900 10000.0
0.5
1.0
Inte
nsity (
no
rma
lized
)
Wavelength (nm)
Retrieved Measured
(d)
Measured
Reconstructed
Fre
que
ncy
Fre
que
ncy
Time
Time
Results
• 0.6 mJ, 6.2 fs pulses by Hollow Core/Chirp compressor technique
• Scaling up the pulse energy by a factor of 1.5 by using circular input
• Demonstration of measurement of sub-10 fs pulses with SHG-FROG
Further possibilities
Obtaining even higher energy and a shorter pulse
• By lowering gas pressure and further increasing input energy
• By using Ne gas instead of Ar• By improving the compressor technique to
compress a broader spectra