golf. summary group overview operating laser systems research and development outlook
TRANSCRIPT
GOLFGOLF
SummarySummary
Group overviewGroup overview
Operating laser systemsOperating laser systems
Research and Development Research and Development
OutlookOutlook
Group overviewGroup overview
Directeur Ph. Balcou (DR)Adjoints au Directeur
H. Bachau (DR) et V. Tikhonchuk (PR)
R. Bouilleau (AI)A. Filippov (IE)A. LeGoff (AI)L. Merzeau (T)D. Briand (T)
Loic Baucher (IE)
Sources X, Plasmas et ions
H. Jouin (PR)F. Dorchies (CR)
C. Stenz (PR)C. Fourment*
S. Hulin*O. Peyrusse*
S. Jéquier (MC)B. Pons (PR)
J. Santos (MC)
Plasmas chauds et denses
V. Tikhonchuk (PR)G. Schurtz*
J. Breil*B. Dubroca**
J.-L. Feugeas*P. Nicolai*
M. Olazabal*L. Hallo*
P.-H. Maire*X. Ribeyre*
E. d’Humières (MC)
Équipes de Recherche
Équipes de Recherche
Technologie et supportTechnologie et support
Harmoniques XUV
et applications
P. Martin (CR)H. Bachau (DR)
E. Constant (CR)B. Fabre (MC)G. Geoffroy*
Y. Mairesse (CR)E. Mevel (PR)
Groupe optique etLasers femto
E. Cormier (MC)D. Descamps*C. Medina (AI)
S. Montant*S. Petit (IR)
Groupe PEPSI
L. Hallo*C. Fourment*G. Geoffroy*
G. Malka (MC)Ph. Alasimone (T)
Secrétariat / GestionSecrétariat / Gestion
S. Aussel (T)M. Mondolfi (T)
F. Catelle***
M à D AlphaNov : J. Lopez (IR)
Group members: permanent staffGroup members: permanent staff
Eric CormierA. Prof., HDR
Dominique DescampsCEA Engineer
Capucine MédinaCNRS AI
Sébastien Montant CEA Engineer
Stéphane PetitCNRS IR
Group members : Postdocs and Phd Students Group members : Postdocs and Phd Students
Loic Meignien
Johan Boullet
François Labaye
Coralie Fourcade-Dutin Marie-Christine Nadeau
Julien Nillon Guillaume Machinet
Christophe Hazera
Group responsibilitiesGroup responsibilities
I) Operate and I) Operate and develop the laser develop the laser infrastructuresinfrastructures
II) Research and development in optics II) Research and development in optics and lasers: and lasers:
ultrafast and ultrashort sources ultrafast and ultrashort sources
Group StructureGroup Structure
Laser systems maintenance and evolutionLaser systems maintenance and evolution
Research and developments in optics and lasersResearch and developments in optics and lasers
Dominique
70 %
30 %
Capucine
80 %
20 %
Stéphane
70 %
30 %
Eric
50 %
Sébastien
100 %
Man power : 2.2
Man power (permanent): 2.3
Postdocs (2)
And
Phd (6)
Total man power : 10.3
SummarySummary
Group overviewGroup overview
Laser infrastructuresLaser infrastructures
Research and Development Research and Development
OutlookOutlook
Laser infrastructuresLaser infrastructures
Group missionsGroup missions• Daily operation of Aurore (1 kHz) and Eclipse (10 Hz) laser facilities • Install online diagnostics for permanent monitoring• Upgrade the laser performances (COLA project)• Access:
• National (5 weeks/year) • European (8 weeks/year)
Human resources and beamtimeHuman resources and beamtime
2005 2006 2007 2008 20090
5
10
15
20
25
30
35
40
45
Bea
mtim
e (w
eeks
)
Years
Aurore Eclipse 100 Hz Eclipse 10 Hz
2005 2006 2007 2008 20090
1
2
3
4
Ma
np
ow
er
(nu
mb
er
of
pe
op
le)
Years
assistant engineer researcher
Move to new building
Aurore upgrade(2 beams)
Eclipse operating(2 beams at 10 Hz)
Eclipse underconstruction
Aurore facilityAurore facility
PC Picker1 nJ-270 ps
PC CleanerTi:sapphire
oscillator 20 fs
Nd:YLF1 kHz 15W
Regenerativeamplifier
1.8 mJ
180 ps
7 mJ-35 fs 1 kHz
Öffner strecher
Nd:YLF1 kHz 29W
Nd:YLF1 kHz 29W
Nd:YLF1 kHz 29W
Nd:YLF1 kHz 29W
7 mJ-35 fs 1 kHz
Cryogenic multipassamplifier
Laser specifications:Laser specifications:
- Repetition rate : Repetition rate : 1 kHz1 kHz- Bandwidth : - Bandwidth : 30 nm FWHM @ 30 nm FWHM @ 810 nm810 nm - Pulse duration : - Pulse duration : 35 fs35 fs FWHM FWHM- Energy : - Energy : 2 x 7 mJ2 x 7 mJ- Temporal contrast : - Temporal contrast : Prepulse at 8 ns ~ Prepulse at 8 ns ~ 6 106 10-8-8
ASE level ~ ASE level ~ 3 103 10-8-8 - Intensity on target : - Intensity on target : 7 107 101616 W/cm W/cm22 (with f=200 mm) (with f=200 mm)- Energy stability : - Energy stability : ± ± 1,4% rms1,4% rms shot to shot shot to shot
22 mJ 1 kHz
TOPAS (1.2-2.2 m)
600 J-50 fs 1 kHz
Compressor Compressor
Laser room +
3 Experimental areas
Eclipse facilityEclipse facility
Laser specifications:Laser specifications:
- Repetition rate : Repetition rate : 10 Hz10 Hz- Bandwidth : - Bandwidth : 28 nm FWHM @ 28 nm FWHM @ 812 nm812 nm - Pulse duration : - Pulse duration : 40 fs40 fs FWHM FWHM- Energy : - Energy : 170 mJ170 mJ- Temporal contrast : - Temporal contrast : Prepulse at 12 ns ~ Prepulse at 12 ns ~ 4 104 10-9-9
ASE level ~ ASE level ~ 1010-7-7 - Intensity on target : - Intensity on target : 2 102 101818 W/cm W/cm22 (with f=250 mm) (with f=250 mm)- Energy stability : - Energy stability : ± ± 5,1% rms5,1% rms shot to shot shot to shot
Multipass amplifier
PC cleanerTi: sapphire
oscillator 20 fs
Nd:YAG100Hz 4W
Regenerative amplifier
Multipassamplifier
1 mJ8 mJ
Nd:YAG10Hz 10 W
300 mJ
10 Hz
Öffner strecher
PC picker1 nJ-270 ps
Laser room +
3 Experimental areas
5 mJ-40 fs 100 Hz
170 mJ*-40 fs 10 Hz
Compressor in air
Compressorunder vacuum
*present configuration 2 beams of 85 mJ
GOLF impact on the other groups GOLF impact on the other groups
TW systems are the heart of the experimental research TW systems are the heart of the experimental research at CELIA at CELIA We manage now to provide distributed beam lines We manage now to provide distributed beam lines allowing allowing 5 to 6 experiments5 to 6 experiments in parallel in parallelHigh productivity of the experimental groups relies on High productivity of the experimental groups relies on our ability to reliably run the systems on a daily basisour ability to reliably run the systems on a daily basisFuture CELIA laser sources will emerge from our Future CELIA laser sources will emerge from our reseachreseach
High implication of 3 out of the 5 members of the groupHigh implication of 3 out of the 5 members of the group
High pressure on the group members
SummarySummary
Group overviewGroup overview
Laser infrastructuresLaser infrastructures
Research and DevelopmentResearch and Development
OutlookOutlook
Research areas and strategyResearch areas and strategy
FiberFiber lasers and amplifiers:
fs, ps, ns and cw
BulkBulk Ti:Sapphire and
new materials
Non linearNon linear optics:OPA/OPCPA
Post-compression
DiagnosticsDiagnostics:Spider, FROG,
wavefront, contrast
ApplicationsApplications:HHG @ 1 MHzExternal Fabry Pérot cavity enhancementUltrafast micro machiningTunable IR sources (600nm – 2.5 µm)Tunable HHGHighly non-linear fiber characterization …
Future CELIA facilitiesFuture CELIA facilities
Research axis Research axis
Ultrashort pulsesUltrashort pulses Ultra high repetition rateUltra high repetition rate
Research axis Research axis
Ultrashort pulsesUltrashort pulses Ultra high repetition rateUltra high repetition rate
PostCompres.
OPCPA Fiber lasers
fs
FP Cavity
psns cw
bulk
Research axis Research axis
Ultrashort pulsesUltrashort pulses Ultra high repetition rateUltra high repetition rate
PostCompres.
OPCPA
10 m
J 10
fs
Low
ene
rgy
Oct
ave
span
.
10fs
100
kHz
CE
P s
elf
stab
.
Fiber lasers
fs
FP Cavity
psns cw
bulk
HH
G
µ m
achi
ning
30 W
270
fs
100
W,9
77nm
1mJ,
977n
m
X-r
ay
Pol
ar. -
ray
Research axis Research axis
Ultrashort pulsesUltrashort pulses Ultra high repetition rateUltra high repetition rate
PostCompres.
OPCPA
10 m
J 10
fs
Low
ene
rgy
Oct
ave
span
.
10fs
100
kHz
CE
P s
elf
stab
.
Fiber lasers
fs
FP Cavity
psns cw
bulk
HH
G
µ m
achi
ning
30 W
270
fs
100
W,9
77nm
1mJ,
977n
m
X-r
ay
Pol
ar. -
ray
WR
Int.
Col
., W
R
Pat
.
WR
, P
at.
WR
, P
at.
Indu
s.
Int.
Col
.
Indu
s.
Indu
s.
WR
Research axis Research axis
Ultrashort pulsesUltrashort pulses Ultra high repetition rateUltra high repetition rate
PostCompres.
OPCPA
10 m
J 10
fs
Low
ene
rgy
Oct
ave
span
.
10fs
100
kHz
CE
P s
elf
stab
.
Fiber lasers
fs
FP Cavity
psns cw
bulk
HH
G
µ m
achi
ning
30 W
270
fs
100
W,9
77nm
1mJ,
977n
m
X-r
ay
Pol
ar. -
ray
WR
Int.
Col
., W
R
Pat
.
WR
, P
at.
WR
, P
at.
Indu
s.
Int.
Col
.
Indu
s.
Indu
s.
WR
Spin off company
Product line of Amplitude Systèmes
Societal applications
#1 High energy post-compression using gas ionization#1 High energy post-compression using gas ionization
Gas ionization =Gas ionization = plasma creation : plasma creation : time evolution of free electron density (ne)time evolution of free electron density (ne)
Temporal phase :Temporal phase :new frequenciesnew frequencies
1/ 20
0
( )2( ) (1 ) *e
c
n tt t L
n
-150 -100 -50 0 50 100 150600
700
800
Wavelength
Wav
elen
gth
(n
m)
Time (fs)
Broadened and blue-shifted spectrum
ADK model P=1 mbar HeI= 2.1015W/cm2 (40 fs) L=40 cm
-150 -100 -50 0 50 100 1500
1
2
3
Intensity
Inte
nsit
y (
101
5 W/c
m2 )
Time (fs)
0
1
2
3
Ele
ctr
on
den
sit
y (
101
6 e/c
m3 )
ne
0%
100%
30fs
ne=2.4 1016 e/cm3
#1 High energy post-compression using gas ionization #1 High energy post-compression using gas ionization
0 1 2 3 4 5 6 7 8 90
5
10
15
20
25
30
Transmitted energy
Out
put e
nerg
y (m
J)
Helium pressure (mbar)
0
5
10
15
20
25
30
35
40 Pulse duration
FW
HM
of p
ulse
dur
atio
n (f
s)
Coupling efficiency 36%
He gas Ein = 70 mJ
Eout= 25.6 mJ (without gas)
Propagation in the capillary (Φcapillary = 420 µm)
40cm
Intensity in the capillary : 2 1015 W/cm2
Spectrum at different He pressure Output energy and pulse duration
11.4 fs11.4 fs
13.7 mJ13.7 mJ
650 700 750 800 8500,0
0,5
1,0
1,5
0 mbar 1 mbar 3 mbar 8 mbar
Inte
nsi
ty (
arb
.u.)
Wavelength (nm)
Coll. XUV Group
Coll. XUV Group
#2 Ultra high repetition rate HHG#2 Ultra high repetition rate HHG
Up to 30 WUp to 30 W
280 fs280 fs
100 KHZ – 1 MHz100 KHZ – 1 MHz
Fiber CPA systemFiber CPA system
Gas jetGas jet
XUV gratingXUV gratingCCD CCD Camera
Camera
Fiber laser systemFiber laser system Tight focusingTight focusing chamber chamber
#2 Ultra high repetition rate HHG#2 Ultra high repetition rate HHG
33.2 nm
1 MHz68.7 nm
FWHM = 280 fs
M2 = 1.3
100 kHz
Rod type fibers
#2 Ultra high repetition rate HHG#2 Ultra high repetition rate HHG
First demonstration of HHG driven by a FCPA systemCoherent radiation down to 33 nm (40 eV) XUV pulses at rep. rate up to 1 MHz System is tunable from 100 kHz to 1 MHzSystem perfectly adapted for pump probe experiments
Move synchrotron based applications to table top
experimentsRevisit the Ti:sapph based HHG
experiments at MHz repetition rates
Patent pending
Patent pending
#3 #3 Few cycles pulses at 100 KHzFew cycles pulses at 100 KHz
Strong driving laser:
Yb Fiber
Post-compressionCapillary
= 50 fs
OPA/NOPA/OPCPA
= 450-1000 nm E = 0.01 – 100 µJ
= 200 nm
< 10 fs
High repetition rate High intensityFew cycle pulsesCEP stabilized
Fiber pumped OPCPA
#3 #3 Few cycles pulses at 100 KHzFew cycles pulses at 100 KHz
CEP stabilized
Modelocked source
Signal stretcher
Yb Fiber CPA pump
Parametric amplifiers
Compressor
25 pJ @1030 nm
60%
25 pJ @1030 nm
60%
Rainbow
• 7 fs Ti:Sapph Oscillator• 300 nm @ -10dB• CEP stabilized
Signal Pump
20 pJ @ 1030
#3 #3 Few cycles pulses at 100 KHzFew cycles pulses at 100 KHz
• Spectrum • Duration
68 nm amplified bandwidth @ 720 nm11 fs (3.6 cycles)
-40 -30 -20 -10 0 10 20 30 40
0.0
0.2
0.4
0.6
0.8
1.0
field = 10 fs
Auto
corr
ela
tion
time (fs)
autoco = 14,1 fs
fs
field
fs
650 700 750 800 850 900
0
50
100
150
200
250
300
Sp
ectr
e
(a.u
.)
Wavelength (nm)
Experiment Gaussian Fit
= 68 nm
nm
SummarySummary
Group overviewGroup overview
Laser infrastructuresLaser infrastructures
Research and Development Research and Development
OutlookOutlook
Laser infrastructuresLaser infrastructures
Aurore (1 KHz)Aurore (1 KHz) Increase average power up to 35 W (additional Ti:sapphire amplifier)
3 x 8 mJ or 1 x 25 mJ3 x 8 mJ or 1 x 25 mJ (2010) Reduce pulse duration down to 25 fs (new oscillator + spectral filter +
dazzler)1 TW – 1 kHz1 TW – 1 kHz laser (2010)
Few cycle pulses at 2 µm using post-compression of TOPAS system (2010)
Eclipse (10 Hz)Eclipse (10 Hz) Improve energy stability (stabbler) (2010) Temporal contrast enhancement up to 1010 (XPW filter+double CPA)
(2012) Reduce pulse duration down to 30 fs (spectral filter + Dazzler) (2012)
Research and DevelopmentsResearch and Developments
High energy CEP stabilized OPCPAHigh energy CEP stabilized OPCPA
High brightness optical pumping of YbHigh brightness optical pumping of Yb
CEP stabilized few cycles at 100 KHz CEP stabilized few cycles at 100 KHz (Solstice)(Solstice)
Fiber lasers at 2 µmFiber lasers at 2 µm
Passive FP cavitiesPassive FP cavities
X-rays and X-rays and -rays via Compton scattering -rays via Compton scattering
-ray production-ray production
e-
h
(1) Low emittance e- source
ATF @ KEK
(2) High finesse FPcavity
4-mirror @ LAL
(3) High power laser
fiber laser @ CELIA
-ray production-ray production54 m
30 m
Beam Energy
→ 1.28GeV
Beam Size
→ 100μm×10μm
Emittance →
1.0x10-9 rad.m
1.0x10-11 rad.m
(Ultra Low !!)
Fiber laser and FP cavity
Technology transferTechnology transfer
Group overview (extra)Group overview (extra)
Group members turn overGroup members turn over
ContractsContracts
Total :Total : 3 M€ 3 M€
Scientific productionScientific production
Active permanent man power dedicated to Active permanent man power dedicated to research: 2.3research: 2.3
ACL / man power = 17 papers / per person