solid-state laser technology · university of central florida college of optics & photonics •...
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![Page 1: Solid-State Laser Technology · University of Central Florida College of Optics & Photonics • CREOL • FPCE 11th Advanced Accelerator Concepts Workshop Stony Brook New York, June](https://reader033.vdocument.in/reader033/viewer/2022042320/5f0987387e708231d427417f/html5/thumbnails/1.jpg)
University of Central FloridaCollege of Optics & Photonics • CREOL • FPCE
11th Advanced Accelerator Concepts WorkshopStony Brook New York, June 22nd, 2004
Solid-State Laser Technology
Prof. Craig W. [email protected]
College of Optics & Photonics / CREOL-FPCEThe University of Central Florida
Orlando FL
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
College of Optics & Photonics / CREOL-FPCE
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
College of Optics & Photonics / CREOL-FPCE
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Historical Introduction
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
History: The Golden Age of Lasers
May 17, 1960: The Beginning. Ted Maiman’s Ruby Laser.Nature 187, 493 (August 6, 1960).
• Nd:glass optical fiber laser: Snitzer, PRL 7, 444(1961).• Q-Switched Laser: Hellwarth, Bull. Am. Phys. Soc. 6, 414 (1961).• GaAs laser diode: GE, IBM, Lincoln Labs,1962.• Modelocking, 1963.• Nd:YAG laser, 1964.
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Early SSL Applications
Compliments A. Siegman
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New materials, techniques provide unprecedented laser intensities ...Big Science
Big Science
Small LabSmall Labin thein the
year1960 1970 1980 1990 2000
1015
1010mode-lockingQ-switching
Relativistic nonlinear optics LWFA+
1010
1012Non perturbativenon linear optics
Chirped Pulse Amplification (CPA)
Perry & Mourou, Science 264, 917 (1994).
CWS Starts PhD w/ MCD
CWS Finishes PhD
Focused Optical Field (V/m)
FocusedIntensity(W/cm2)
1020
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Chirped Pulse Amplified Laser System
UCSD 20UCSD 20--Hz, 20Hz, 20--fs fs 55--TW Laser SystemTW Laser System
•• CompactCompact•• Ultrafast Ultrafast –– 20 20 fsfs•• Ti:SapphireTi:Sapphire•• Synchronous Synchronous
Pump & ProbePump & Probe•• 100 100 mJmJ @ 20 Hz@ 20 Hz
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Chirped Pulse Amplification
Inverse delay line
t
t
Solid state amplifiers
!! Saturation is Reached Safely:Saturation is Reached Safely: IIpeakpeak << << IIdamagedamage
t
Dispersive delay line
Strickland & Mourou, Opt. Comm. 56, 219 (1985).Cook, Proc. IRE, 310 (1960).
!! Peak Power Increase Proportional toPeak Power Increase Proportional to
t
Short pulse oscillator
∆tstretch = Fsat/IdamageNd:Glass ~ 1 ns Ti:Al2O3 ~ 200 ps
10000
stretch >>∆
∆t
t
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Disperse-O-Matic Freeware(WARNING: Shameless Self-Promotion)
http://dom.creol.ucf.edu/ http://www.creol.ucf.edu/reu/
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Chirped Pulse Amplified Laser System
UCSD 20UCSD 20--Hz, 20Hz, 20--fs fs 55--TW Laser SystemTW Laser System
•• Ti:SapphireTi:Sapphire•• 800800--nmnm•• 100100--mJ / pulsemJ / pulse•• Excellent focusingExcellent focusing•• 10101818 W/cmW/cm22
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Ultrafast CPA CharacteristicsCompactness and high repetition rateCompactness and high repetition rate
NovaNovaPulse duration 1 ns10 kJ/beam10 TW/beam1 shot/hour
UltrafastUltrafast CPA SystemCPA SystemPulse duration 20 fs100 mJ/beam5 TW/pulse72,000 shots/hour
UltrafastUltrafast CPA systems allow high experimental “Utility”CPA systems allow high experimental “Utility”•• Signal averaging even at extreme intensitiesSignal averaging even at extreme intensities•• High average flux of laserHigh average flux of laser--generated xgenerated x--rays, particlesrays, particles
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Big Science in the Small Laboratory
HighHigh--fluxflux~10~10--keV xkeV x--raysrays
HighHigh--fieldfieldHighHigh--reprep--raterateUltrafast lasersUltrafast lasers
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Even Bigger Science in the Big LabJAERI Petawatt
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
SAUUL Report: >10TW Facilities
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
SAUUL Report: PW Facilities
UT Austin 1PW Nd:glass 160fs 130J Under Construction
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
What We Care About
18 2osc0 1 or 10 W/cmva I
c= ≈ ≈
Laser Sources WG, AACW ‘96
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Pulse Duration
Agostini & DiMauro, Rep. Prog. Phys. 67 813 (2004).
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Average Power Challenge
• Traditional USP lasers are limited to watt-level average powers.
• Transitioning of short pulse high-intensity applications require kW-level USP lasers. mW
kW
W
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Efficiency & Saturation Perspective
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Saturation Fluence
σ
hν
sathF νσ
=
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Efficient Solid-State Amplifier
• High Efficiency in Final Amplifier– Operate above the saturation fluence
Fsat
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Nd:YVO4
Nd:YAG
Nd:YLF
Er:Glass
Cr:ForsteriteCr:LiSAF
Nd:Glass Fsat ~ 5 J/cm2
Ti:Sapphire
Fsat ~ 1 J/cm2
Cr:YAG
Cr:LiCAFEr:YAG
Yb:YAGYb:Glass
Fsat ~ 30-50 J/cm2
RG6 & SemiconductorsFsat ~ 1 mJ/cm2
Compactness & Saturation Fluence
High Fsat materialscan be more compact.
1-J Beam Areas at Fsat
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Saturation Intensity
0 2 4 6 8 10t @nsD5
10
15
20
25
30
niaGBd
5.9 5.95 6 6.05t @nsD5
10
15
20
25
30
niaGBd
Gain recovery time τ
satsat
F hI ντ στ
= =
CW-Pumped Pulse Amplifier
6.1
0 2 4 6 8 10t @nsD0
200
400
600
800
1000
ni_I,
tuo_IWM
mc2
5.9 5.95 6 6.05 6.t @nsD0
200
400
600
800
1000
ni_I,
tuo_IWM
mc2
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Energy Considerations in USPs
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Laser Media
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Damage Fluence Limits
Ultrashort-pulse damage thresholds limit usable fluences.
Dielectrics
Metals
B. Stuart, et al., JOSA B 13, 459 (1996); ibid, PRL 74 (1995).Pronko, Opt. Comm. 114, 106 (1995).
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Laser Media
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Optical Damage Limits
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
eXtreme Chirped Pulse Amplification
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XCPA Semiconductor AmplifierLimits ASE & Nonlinearities
Solid-State Ampcompressed
Single-pulse CPAstretched
SOA gainsub-µs to ms
compressed
50-MHz pulse train stretched to ~ 20ns
Burst modeXCPA
SOA operated as CW amplifier.
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
eXtreme CPA
10 100 1000 10000G0 I_in @MW�cm2D
0.1
1
10100
100010000
tuo_F-
ni_FJm
mc2
500 1000 10
0.11
10100
100010000
tuo_F-
ni_FJm
mc2
10000�D 10 100 1000 10000G0 I_in @MW�cm2D
10205000ytisnetnI 10
100
tuo_I-
ni_I
Pulse Durations: 2-ps (red), 20-ps (yellow), 200-ps (green), 2-ns (blue), 20-ns (violet)
200-ps gain lifetime, 30-dB gainFsat = 1.0-mJ/cm2; Isat = 5.1 MW/cm2
λ = 980-nm; σ = 2.5x10-16 cm2
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Optical Damage Limits
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Thermal Damage Limits
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Sub-0.5ps Materials
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
High-power laser diodesLightStack from Coherent
2-kW @ 940-nm. 50% wallplug efficiency2 19-bar arrays in series electrically, parallel cooling
Pump Stack Originally developed for Ytterbium Fiber Pump
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
High-power laser diodes
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Sub-0.5ps Materials
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
High-Power Diode Pump-able
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
What We Care About
18 2osc0 1 or 10 W/cmva I
c= ≈ ≈
Laser Sources WG, AACW ‘96
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Systems Which Access AAC-Relevant Rep-Rates
Saturated Rep-Rate [kHz]10-1 100 101 102 103
Sat
urat
ion
Flue
nce
[J/c
m2 ]
10-4
10-3
10-2
10-1
100
101
102
103
Ti:Sapphire
Cr4+:CUNYite
Cr4+:YAG
Alexandrite
Co:MgF2Yb:Glass
Er:Glass
Cr4+:Forsterite
Nd:GlassYb:YAG
Yb:KGW
Nd:KGW
Nd:Vanadate
Nd:YLF
Nd:YAG
AAC
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Energy Storage Density
Energy Storage Density [J/cm3]10-1 100 101 102 103 104
Satu
ratio
n Fl
uenc
e [J
/cm
2 ]
10-4
10-3
10-2
10-1
100
101
102
103
Ti:Sapphire
Cr4+:CUNYite
R6G
Cr4+:YAG
Alexandrite
Co:MgF2Yb:Glass
Semi
Er:Glass
Cr4+:Forsterite
Nd:GlassYb:YAG
Yb:KGW
Nd:KGW
Nd:Vanadate
Nd:YLF
Nd:YAG
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Nd:Glass
• Energy storage good – Fsat = 7 J/cm2
• Pumping straightforward– 400 microsecond lifetime
easily flashlamp pumpable• Dispersion control easier
– Picosecond pulses require only GDD and maybe cubiccompensation
• Repetition limited– Thermal loading a problem. Must wait to re-equilibrate
• Pulse duration limited to around a picosecond– Typically 300 fs to 1 ps
• First PW Laser – LLNL/NOVA PW• Majority of planned PW’s are Nd:Glass
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UCF College of Optics & Photonics/CREOLUCF College of Optics & Photonics/CREOL--FPCEFPCE
Yb:Glass• High energy storage
– Fsat = 30-50 J/cm2
– Damage is a major issue in efficiency and robustness• Diode pumpable
– Very long lifetime (840 µs) and absorption at diode wavelengths (915nm, 980nm). Not optimal for 10-100kHz rep-rate applications.
• Shorter pulses possible– Fluoresence bandwidth should support ~100 fs
• Stretching requirements difficult - CFBG?– ∆t = 6ns to reach one times saturation safely
• Can be easily implemented in Fiber geometry– >kW CW average powers, 65% slope efficiency demonstrated (Limpert
CLEO ‘04)– 0.6-mJ, 1.6-kHz, 800-ps stretched, 400-fs compressed (Limpert CLEO ‘04)
• Yb:glass PW’s under construction• Yb:SFAP - Mercury Laser @ LLNL. 100J, 10 Hz, ns.
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Ti:Sapphire
• Sapphire great optical quality, high damage threshold– Also superior thermal material. Sapphire is often used as
transparent heat sink • Ideal saturation fluence
– Fsat = 1 J/cm2 yields a stretching requirement of only 200 ps– Just below damage threshold
• Huge bandwidth– Theoretically could support 3-fs pulses
• Short lifetime– 3 us requires laser pumping or heroic flashlamp circuitry
• SHG-Nd pumping. No high-power green laser diodes.• Widely implemented for 1-100 TW class systems.• PW’s: JAERI, FOCUS
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Cr4+:YAG
• Versatile Pumping– Diode-pumped @ 940-nm, 980-nm– Laser-pumped by Nd, Yb lasers
• Operates at telecomm wavelengths (1.3 and 1.5um)• Excellent optical quality material available (Passive Q-
Switch Use)• Ideal saturation fluence
– Fsat ~ 0.5 J/cm2 yields a stretching requirement of only 100 ps– Just below damage threshold
• Large bandwidth– Theoretically could support sub-10 fs pulses
• Short lifetime– 4.5 us requires laser pumping– High rep-rate pulsed amplifier for 10-100 kHz applications
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Er:fiber
• Telecom wavelengths: much hardware available– EDFA: The most common telecommunication fiber amplifier
• All diode pumped• Short pulses
– 100 fs possible
• Large scale hosts not available so limited energy out• Reliable source of sub-100-fs pulses at 1550nm.• Sub-MW peak powers: TW/cm2 at 10’s MHz rep-rates
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OPCPA?
(T. Ditmire)
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Cr:LiSAF
• Flashlamp pumpable and diode pumpable– 67 µs lifetime, absorption at diode wavelengths– Diode pumped fs oscillators have been made with this material
• Good but not best bandwidth– Theoretically around 10 fs
• Inferior material properties– Early crystals dissolved in their water cooled housings– Easily fractured
• Inferior optical quality
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Pros & Cons of Amp Shape
Thermal DistortionsAperture limit & beam combining. USP nonlinearities. ASE.
Mode, Mode, and ModeThermal Lensing & ModeKey Challenge
13 kW, M2 ~ 41.3 kW, M2 ~1.33 kW, M2 ~ 2.5500 W, M2 ~ 1.5Best Power with good Beam Qual
Up to 95%~100%Up to ~80%Up to ~80%Mode Fill Factor (TEM00)
GoodGood for single mode. More challenging for large mode fibers.
Challenging, especially at large aspect ratios.
Good at low power.Mode Control
Minimal due to 1D heat flow.
None for glass fibers.None in ideal case.Significant, but can be dealt with.
Stress Birefringence
Minimal due to 1D heat flow.
Significant, but can be dealt with.
None in y-z (zigzag averaging), weak in x-z.
Significant, but can be dealt with.
Thermal Lensing
DiskFiberZigzag SlabRod
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What Does the Future Hold?
• Diode-pumped Fiber Osc’s & Amps: – Yb (1um), Er (1.5um)– High rep-rates, limited by USP NLO
• Disk Amps: Yb, Cr4+
• X-CPA & SOA’s• Nano-photonics & Integrated Optics• Dispersion Management
– Improved Gratings (~J/cm2 Damage Thresh.)– Chirped Fiber Bragg Gratings– Compact Free-Space Systems
• Engineered Composite Media– Large-area “crystals”: ceramic, fused, etc.– Thermal Management Improvements (because we must!)
• Multi-kW, Multi-kHz USPs soon!• GHz GW and MHz TW?
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X-CPA Generic Architecture
Modelocked Laser
Pre-Stretch~100 psec
Primary Stretch – 20 nsec Primary Compress
Primary Optical Amplification
Pre Optical Amplification
Final Compression
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DARPA Challenge
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Stu’s Shoe
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DARPA Challenge
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Size Reduction Obtainable from XCPA
Traditional mode locked laser for Ti:Sapphire USPL (KM Labs, Boulder).
46 inches
10inches
A packaged mode locked laser diode X-CPA USPL
1 inch
0.5 inch
This is the laser diode based Mode locked laser to the same scale as the traditional modeLocked laser for a Ti Sapphire
2760 in3 for the volume for the traditional Ti Sapphire ML source 0.125 in3 for the ML source for the X-CPA
22080 time reduction in volume
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X-CPA Impact
10in
14in8in
48in24in
9in=
Volume 10368in3 for a 1 Watt Ave PowerTi:Sapphire Power Supply and Water cooling
system are not shown in the photograph Volume 1120in3 for a 0.5 Watt Ave Power
XCPA Power Supply not shown.
Volume of power supply ~560in3
Water Cool Not RequiredVolume of power supply 3456in3
Volume of water cool 3000in3