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![Page 1: Laser Source for the - Collider Jim Early Lawrence Livermore National Lab Laser Science and Technology SPLAT Short Pulse Lasers, Applications & Technology.](https://reader036.fdocuments.us/reader036/viewer/2022062409/56649f115503460f94c23d50/html5/thumbnails/1.jpg)
Laser Source for the - Collider
Jim EarlyLawrence Livermore National LabLaser Science and Technology
SPLATShort Pulse Lasers,
Applications & Technology
Presented to: Snowmass 2001 July 6, 2001
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Requirements for gamma-gamma laser LLNL
• Efficient conversion of electron energy to photons requires:
- laser wavelength near 1m
- laser pulse duration near 2ps to overlap electron pulse
- 1J per subpulse in high quality beam for adequate photon density in
conversion zone
- laser pulse format matching electron accelerator
• Low duty factor and short pulse duration requires use of “storage” laser
- solid state storage lasers used in laser fusion program give ns pulses
- thermal management of high average power a challenge in solid lasers
• Optical compression required to avoid damage in laser amplifier
- pulse must be stretched from several ps to several ns before amplifier
- chirp pulse stretching and compression technique required
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Laser architecture driven by electron bunch format
96 pulses1J, 2ps, 1 m
3ns spacing
120 Hz macro-pulses
• 100 J macro-pulses require large “storage” laser amplifier
• Amplifier thermal design leads to low, 10 Hz, laser pulse rate
- 12 amplifiers use simple spatial combiner to achieve 120 Hz
• DOE Inertial Fusion Energy program developing “Mercury” laser that
meets requirements
• Optical design breaks 100 J macro-pulse into train of 1 J sub-pulses
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laser system architecture: CPA front endseeds 12 Mercury power amplifiers
Mode-lockedoscillator
Spectral shaper
Stretcher OP-CPApreamp
Mercury power ampMercury power amp
Mercury power amp
Beamsplitters
12- 100 J power amplifiers
Optics:Combiner, splitters
Grating compressor 100 J macropulse:100X 2ps micropulses120 Hz
0.5 J3 ns120 Hz
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Goals:• 100 J • 10 Hz• 10% electrical • 2-10 ns
The Mercury laser will utilize three key technologies: gas cooling, diodes, and Yb:S-FAP crystals
vacuum relay
gas-cooledamplifier head
Injection and reversor
Architecture: - 2 amplifier heads - angular multiplexing - 4 pass- relay imaging - wavefront correction
front end
DM
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Pump delivery
Front end
Injection multi-pass spatial filter
Diode pulsers
Gas-cooled amplifier head
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Milestone budget breakout:
1. $3030k Build two pump delivery systems
2. $1800k Fabricate Yb:S-FAP crystals
3. $825k Design and build wedged amplifier head
4. $1025k Build injection and reverser hardware
5. $1270k Integrated tests and code benchmarking
6. $300k Advanced Yb:S-FAP growth
7. $350k (LLE) Spectral sculpting experiments and evaluation of
average-power frequency conversion design
Mercury project FY01 funding from IFE program
We are on schedule to build half Mercury in FY01.FY02 funding will be slight increase.
We are on schedule to build half Mercury in FY01.FY02 funding will be slight increase.
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Objective 1: Build two pump delivery systems
beam
diode package on split backplanes
gas-cooledamplifier head
vacuumenclosure
pump duct and homogenizer
Goal
Status
• 80 V-BASIS 23-bar 900 nm tiles fabricated
• Two functioning backplanes loaded with diodes
• Remaining power supplies/pulsers purchased
• Pump delivery hardware assembled, integrated, and currently being activated
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The Mercury diodes deliver the pump light toYb:S-FAP crystals
Half array is madeof 5x7 =35 tiles
Full array 161 kW
4 pairs of half arrayslike these are requiredfor Mercury 644 kW
.
diode
v-sp
ring
Si submount
Mo block
Si lensframe
mic
role
ns
55°
Each tile is madeof 23 diode bars
2.3kW
Diode light distribution (green) obtained in a plane normal to the optical axis
7 tiles
5 tiles
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The V-BASIS packaged diode bars meet the optical specifications of the Mercury Laser System
1 full backplane array (72Mounted tiles) complete
5% droop demonstrated
44% demonstrated
Completed Fabrication of 80 tiles
StatusRequirement
Demonstrated 3.7 nm FWHM on tiles for one split backplane
Pulse integratedLinewidth < 8.5 nm FWHM
Assemble tiles onsplit backplane
Power droop duringpulse < 15%
Testing is ongoing, butcurrently demonstrated1.4 x 108 shots without problems
Reliability of> 2 x 108 shots
45% electrical toOptical efficiency
115 W peak / 1 cm bar demonstrated with good lifetime
100 W peak /1 cm bar
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104
103
102
101
1
0.1 88 90 92 94 96 98 00 02
Copper Heat Sinks
Microchannel Cooled Bars
Microchannel Cooled Monolithic Arrays
CW Bars
Peak Power Bars
Sources: L&O Market Survey 10/93L&O Market Survey 11/95LLNL/USEC Survey 96
Year
$ /W
att
Laser Focus World 2/98Purchase Order 99Quotation for 00 deliveryD. Scifres (SDL) CLEO ‘99
Similar to other integrated circuit technology, the cost of diode arrays has been dropping even while the performance has been increasing
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Heliumgas
Slabmetalvanes
Channelsection
Diffusersection
Nozzlesection
Edge claddingWindow
Gas cooled head and vanes
1/8
0
0.1 Machgas flow
4 atmpressure
static
Pressure and gas flow contributes 1/16 wave to wavefront distortion
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Fabrication of Yb:S-FAP crystals
Goal A full size 4x6 cm amplifier slab
Two 3x5 cm slabs Status
• One full size bonded amplifier slab completed - awaiting polish and AR coating
• Two smaller slabs (usable) also completed and await finishing
• Processes are not completely reproducible at this point
A axis
4 cm
6 cm
C axis
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Crystals of Yb:S-FAP are grown by using theCzochralski (CZ) Method
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Appropriate spectral sculpting of the input pulse can lead to a linearly chirped gaussian output pulse (2 psec stretched output pulse case)
RJB/VG 3-Oct-00 short Pulse Mercury Laser
Extraction Pulse Temporal Profile
0.0E+00
5.0E+09
1.0E+10
1.5E+10
2.0E+10
2.5E+10
3.0E+10
3.5E+10
4.0E+10
-8.E-09 -6.E-09 -4.E-09 -2.E-09 0.E+00 2.E-09 4.E-09 6.E-09 8.E-09
(sec)
(W)
Pass 4 (output)Pass 3Pass 2Pass 1Input Pulse
Normalized Emission Line and Saturated Gain for Yb:S-FAP
00.10.20.30.40.50.60.70.80.9
1
1035 1040 1045 1050 1055 1060
nm
Input Pulse Temporal Profile
0.0E+00
1.0E+06
2.0E+06
3.0E+06
4.0E+06
5.0E+06
6.0E+06
7.0E+06
8.0E+06
9.0E+06
-8.E-09 -6.E-09 -4.E-09 -2.E-09 0.E+00 2.E-09 4.E-09 6.E-09 8.E-09
(sec)
(W)
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Telephoto ImagingSystem
LCM Light Valve
• Gratings: 1740 grooves/mm
• Telephoto imaging system EFL ~ 800 mm
A compact spectral sculptor using a liquid-crystal modulator light valve has been demonstrated
GratingGrating
Inte
nsi
ty
Original FM
Sculpted
0 100 200-100-200
Frequency (GHz)
Inte
nsi
ty
Original FM
Sculpted
0 100 200-100-200
Frequency (GHz)
0 100 200-100-200
Frequency (GHz)
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8 May 1999
New technology enables production of Terawatt to Petawatt (1000 TW) pulses
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Stretcher and compressor gratings LLNL
Stretcher CompressorSubstrate material silica silicaCoating material gold Multi-layerGrating size (cm) 4 x 15 30 x 84Roof mirror size (cm) 4 x 8 (flat) 30 x 40Grating separation (m) 5 15Lines per mm 1740 1740Laser beam diameter (cm) 1 10Cut bandwidth (nm) 2.0 2.0Exit sub-pulse duration (ps) 3000 2.2Efficiency-single bounce (%) 90. 96.0System efficiency (%) 60 80Laser macro-pulse fluence (J/cm2) 10-7 1.3Damage fluence (J/cm2) 0.4 2.0Approximate cost ($K) 20 1400
94 cm aperature gold coated diffraction Multilayer dielectric dielectric gratinggrating used for pulse compression designs of high-index (H) and low-index (L)on the Petawatt laser layers and groove corrugations (G).
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1.00.80.60.40.20.0 -80 -40 0 40 8
0
Amplified pulseautocorrelation
44 fs = 31 fsdeconvolved
Time (fs)
=0.43
Vacuum compressor
0.6 J; 30 fs @ 1 Hz
20 fs Ti:sapphireoscillator
Pulsestretcher
regenerative amplifier: G=10 7
4-pass amplifier: G=40
4-pass amplifier: G=10
3-pass amplifier
45 mJ pump @ 10Hz
280 mJ pump@ 10Hz
1.5 J pump@ 10Hz
4 J pump@ 1Hz
Periscope tolinac caves
Planned upgradeto >7 J
Typical high-power CPA systems use multipleAmplifier stages to obtain gains of 1011
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Optical parametric amplification is based on difference frequency generation
NONLINEAR CRYSTAL
signal
idler
PUMPLASER
short wavelength pump pulse
stretched long wavelengthseed pulse
p
s
i= p- s
ks ki
kp
k
pis kkk
pis
residual pump
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600 mJ pump,532 nm, 8.5 ns
500 pJ seed,1054 nm, 3 ns BBO
preamplifier
vacuum relay telescope I
vacuum relay telescope II
15 %BS
90 mJ
420 mJ
BBO poweramp WP
WP
TFP
TFP
to compressor
31 mJ
0.1 TW-scale OPCPA was demonstrated as a full replacement for regenerative amplifier LLNL
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beam splitter optical delay line
polarizerwave plate
• 100 J macro-pulse from laser converted to train of 1 J subpulses
• Combination of beam splitters and optical delay lines gives two beams
with string of pulses
• Two beams combined on polarizer to give single beam
- alternating linear polarization in pulses
- 96 pulses ( 3 x 25 )
Optical Pulse Train Generation LLNL
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Gamma-gamma laser system cost estimate ($01) LLNL
• Capital costs $M
20 lasers
40 diodes (at $5/W)
10 optics system
20 building
20 development program
_40_ contingency
$150M total
• Operating costs $M/y
8 diodes at $5/W (5y or 109 shot lifetime)
4 labor
4 power
_4_ contingency
$20M/y
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Gamma-gamma laser summary LLNL
• Pulse format of 1m - laser must match electron bunch format
• Mercury laser amplifier under development by DOE can serve as - laser
- laser under construction with single head to be completed in FY01
• New front end for Mercury laser will generate input pulse format needed
• Optical Compression Amplification and use of pulse string generation
optics can modify Mercury pulse format to - requirements
DOE Mercury laser project can serve as the demonstration prototype for the - laser project