Status of High-Power Laser Development at Stanford Shally Saraf*, Supriyo Sinha, Arun Kumar Sridharan and Robert L. Byer E. L. Ginzton Laboratory, Stanford.

Slides:



Advertisements
Similar presentations
Thermal properties of laser crystal Rui Zhang ACCL Division V, RF-Gun Group Feb 20, 2015 SuperKEKB Injector Laser RF Gun Review.
Advertisements

A Scalable Design for a High Energy, High Repetition Rate, Diode-Pumped Solid State Laser (DPSSL) Amplifier Paul Mason, Klaus Ertel, Saumyabrata Banerjee,
Enhanced LIGO Laser System S. Wagner, B. Schulz, R. Wachter, C. Veltkamp, M. Janssen, P. Weßels, M. Frede, D. Kracht.
10W Injection-Locked CW Nd:YAG laser
CNMFrascati 12/01/061 High Power Laser System for Advanced Virgo C.N.Man Design goals Present technology Other activities in the world Virgo+ and Laser.
COMPUTER MODELING OF LASER SYSTEMS
Characteristic evaluation of new laser crystals Rui Zhang ACCL Division V, RF-Gun Group Feb 20, 2015 SuperKEKB Injector Laser RF Gun Review.
CTF3 Laser Status Massimo Petrarca CLIC January
Adaptive Optics for Wavefront Correction of High Average Power Lasers Justin Mansell, Supriyo Sinha, Todd Rutherford, Eric Gustafson, Martin Fejer and.
LIGO-G W 1 Increasing the laser power incident on the recycling mirrors Doug Cook and Rick Savage LIGO commissioning meeting Dec. 22, 2003 Ref.
rd ILIAS-GW annual general meeting 1 VIRGO Commissioning progress J. Marque (EGO)
G D Calibration of the LIGO Interferometer Using the Recoil of Photons Justice Bruursema Mentor: Daniel Sigg.
LSRL 06 Nov, 2003, IAEA CRP Meeting in Vienna Feasibility study on Scalable Self-Phase Locking of two beam combination using stimulated Brillouin scattering.
High-speed optical switching based on diffusive conduction in an optical waveguide with surface-normal optical control V. A. Sabnis, H. V. Demir, M. B.
Stanford Laser Amplifiers for LIGO
LISA symp July 02, PSU 1 Technologies for the Future of interferometric detectors C. Nary MAN UMR 6162, Observatoire Cote d’Azur, BP 4229,
ILE OSAKA New Concept of DPSSL - Tuning laser parameters by controlling temperature - Junji Kawanaka ILE OSAKA US-Japan Workshop on Laser-IFE March.
LSU Amplifier Experiments Rupal S. Amin (LSU) J. Giaime (LSU), D. Hosken (Uni. Adelaide), D. Ottaway (MIT) LSC/VIRGO Meeting March 2007 Lasers Working.
October 16-18, 2012Working Group on Space-based Lidar Winds 1 AEOLUS STATUS Part 1: Design Overview.
LIGO-G Z Gaussian to Super- Gaussian Diffractive Optical Elements Patrick Lu Advisor: Prof. Robert Byer Stanford University March 23, 2005.
Status of the advanced LIGO laser O. Puncken, L. Winkelmann, C. Veltkamp, B. Schulz, S. Wagner, P. Weßels, M. Frede, D. Kracht.
ILIAS WG1 meeting, 19/06/07 IB Faraday Isolator 1 IB in vacuum Faraday isolator E. Genin, S. Hebri, S. Hamdani, P. La Penna, J. Marque EGO.
A 5 fs high average power OPCPA laser system for attosecond pulse production Philip Bates, Yunxin Tang, Emma Springate and Ian Ross Central Laser Facility,
GJ Van der Westhuizen, JP Burger, EG Rohwer, JN Maran Laser Research Institute, Department of Physics, University of Stellenbosch, South Africa NUMERICAL.
CTF3 photo injector laser status CERN 17 July 2009 CLIC meeting.
LIGO-G D Enhanced LIGO Kate Dooley University of Florida On behalf of the LIGO Scientific Collaboration SESAPS Nov. 1, 2008.
R·I·TR·I·T Rochester Institute of Technology -Proposal to join the LSC- Shally Saraf Rochester Institute of Technology Quantum Electronics Group (RITQEG)
B. Willke, Mar 01 LIGO-G Z Laser Developement for Advanced LIGO Benno Willke LSC meeting LIGO-Livingston Site, Mar 2001.
CTF3 Collaboration meeting – CERN, January 2007 Laser system schematic 22 44 1.55  s 200  s, 5-50 Hz 15 kW 10  J 270  s ~2332 pulses 370.
1 Large Aperture Dielectric Gratings for High Power LIGO Interferometry LSC/Virgo Meeting, Baton Rouge March 19-22, 2007 Optics Working Group Jerald A.
Folienvorlagen für Seminarvortrag. Novel laser concepts HR-mirror out coupling mirror disc cooling diode laser focusing optic diode laser focusing optic.
Thermal Compensation in Stable Recycling Cavity 21/03/2006 LSC Meeting 2006 UF LIGO Group Muzammil A. Arain.
Advanced LIGO laser development P. Weßels, L. Winkelmann, O. Puncken, B. Schulz, S. Wagner, M. Hildebrandt, C. Veltkamp, M. Janssen, R. Kluzik, M. Frede,
©LZH M.Frede Aug.02 G Z Status of Laser Zentrum Hannover Laser Program Maik Frede Martina Brendel, Carsten Fallnich, Renê Gau, Philipp Huke, Ralf.
G Z LIGO R&D1 Input Optics Definition, Function The input optics (IO) conditions light from the pre- stabilized laser (PSL) for injection into.
50 W Laser Concepts for Initial LIGO Lutz Winkelmann, Maik Frede, Ralf Wilhelm, Dietmar Kracht Laser Zentrum Hannover LSC March 05 Livingston G Z.
Modeling efforts on the Mercury Laser system Mercury Andy Bayramian, Camille Bibeau, Ray Beach Prop ’92 work: Ron White French Collaboration with MIRO:Olivier.
Advanced Virgo Optical Configuration ILIAS-GW, Tübingen Andreas Freise - Conceptual Design -
©LZH Livingston, La.; LIGO-G Status of 100 W Rod System at LZH Laserzentrum Hannover e. V. Hollerithallee 8 D Hannover Germany.
Stanford High Power Laser Lab Status of high power laser development for LIGO at Stanford Shally Saraf*, Supriyo Sinha, Arun Kumar Sridharan and Robert.
LSC August G Z Gingin High Optical Power Test Facility (AIGO) 1 High Optical Power Test Facility - Status First lock, auto-alignment and.
Min Hyeong KIM High-Speed Circuits and Systems Laboratory E.E. Engineering at YONSEI UNIVERITY
Advancement in photo-injector laser: Second Amplifier & Harmonic Generation M. Petrarca CERN M. Martyanov, G. Luchinin, V. Lozhkarev Institute of Applied.
Development of high-power and stable laser for gravitational wave detection Mio Laboratory Kohei Takeno.
Status of the Advanced LIGO PSL development LSC meeting, Baton Rouge March 2007 G Z Benno Willke for the PSL team.
Status of High-Power Laser Development at Stanford Todd S. Rutherford*, Shailendhar Saraf, Karel Urbanek, Justin Mansell, Eric K. Gustafson, and Robert.
Yb:YAG Regenerative Amplifier for A1 Ground Laser Hut Rui Zhang ACCL Division V, RF-Gun Group Nov 20, 2015 SuperKEKB Injector Laser RF Gun Review.
Phto-injector laser chain NEWS Massimo Petrarca & Marta Divall.
LIGO-G M LIGO R&D1 Initial LIGO upgrade to 30 W: Implication for the Input Optics UFLIGO Group.
Studies of Thermal Loading in Pre-Modecleaners for Advanced LIGO Amber Bullington Stanford University LSC/Virgo March 2007 Meeting Optics Working Group.
LIGO-G Z High Power Components for Advanced LIGO University of Florida Rupal Amin, Joe Gleason, Rachel Parks Christina Leidel, Mike Marquez, Luke.
LIGO Scientific Collaboration Lasers and Optics Working Group 6 Month Report to the LSC - August 15, 2000 Outline Highlights Meeting Agenda LIGO-G D.
THE INPUT OPTICS OF ENHANCED AND ADVANCED LIGO D.B. Tanner, M.A. Arain, A. Lucianetti, R.M. Martin, V. Quetschke, L.F. Williams, Wan Wu, G. Mueller, and.
An H- stripping laser using commercial, diode-pumped Nd:YAG amplifiers Russell Wilcox Laser Stripping Workshop, April 11, 2011.
Optical Engines 842 S Sierra Madre St STE D Colorado Springs CO, (815) Fiber Laser Amplifier Technology.
High power fibered optical components for gravitational waves detector Matthieu Gosselin, PhD Student at EGO ELiTES : 3 rd general meeting February 10.
Laser Adaptive Optics for Advanced LIGO
Absorption Small-Signal Loss Coefficient. Absorption Light might either be attenuated or amplified as it propagates through the medium. What determines.
Yb:YAG Regenerative Amplifier for A1 Ground Laser Hut Rui Zhang ACCL Division V, RF-Gun Group Nov 20, 2015 SuperKEKB Injector Laser RF Gun Review.
NSF Annual Review of the LIGO Laboratory
Light-Matter Interaction
Fiber lasers for GW detectors
Update on the Advanced LIGO PSL Program
Diode Pumped Cryogenic High Energy Yb-Doped Ceramic YAG Amplifier for Ultra-High Intensity Applications P. D. Mason, S. Banerjee, K. Ertel, P. J. Phillips,
Nd:YAG Solid Laser 3-2 / A-1 on the ground
Phto-injector laser chain NEWS
Lasers for Advanced Interferometers
Present status of the laser system for KAGRA
Modeling of Advanced LIGO with Melody
Kansas Light Source Laser System J. R. Macdonald Laboratory
Presentation transcript:

Status of High-Power Laser Development at Stanford Shally Saraf*, Supriyo Sinha, Arun Kumar Sridharan and Robert L. Byer E. L. Ginzton Laboratory, Stanford University LIGO Science Collaboration Meeting Hanford Site, August 19 – 22, 2002 LIGO-G Z

Outline Review of slab lasers. Progress since Livingston LSC. 100W demonstration results. 200W amplifier design and status. (Near) future work.

Rod vs Slab 1 st order thermal lens Spatially dependent birefringence (depolarization) 2 nd order thermal distortions Slightly reduced mode-fill zig-zag slab rod

Face-pumping vs Edge-pumping Pumping Cooling zig-zag plane Pumping Cooling zig-zag plane Face- pumping Edge- pumping zig-zag slab

Nd:YAG Laser Head 3.8 cm

Amplification Goal: 100 W Two zig-zag edge-pumped slab amplifiers. –Brewster ends. –3:1 aspect ratio (width/thickness). About 900 W total pump power. 10W LIGO laser followed by an external amplifier provides 20W to drive slab amplifiers.

Experimental Setup for 100W demonstration 10W LIGO LASER ISOL 20W AMP DUMP Power Meter PB S Edge Pumped Slab #1 Edge Pumped Slab #2 Beam Waist ~ 300  m DUMP

100W experimental setup

10W Amplifier

Increased NPRO power from 235mW to 418mW by turning up drive current from 1.89A to 2.4A. Realigned optical train. Output power increased to 10.4W back to original specs. Set diode temperature to 24.1 o C and pump current to 23A for the double passed amplifier. 10W Amplifier upgrade

20W Amplifier Replaced Faraday Isolator following 10W LIGO Laser. Replaced faulty power supply for external 20W amplifier. Mode matched beam into 20W amplifier (waist ~ 245  m)

Beam quality after 20 W amplifier Measured output power ~ 24.4W.

Edge pumped slab head assembly

Slab 2 power amplifier set up

Complication ---- Slab #1 cracked

Results for slab amplifier # 1 Output Power = Input Power + Extracted Power

Power and M 2 measurement after slab #1 Output Power from triple passed slab #1 = 39W

Slab #2 single pass power output

Slab #2 triple pass power output Power out of MOPA ~ 71.8W

Thermal lens measurements Pumping Cooling zig-zag plane

Future work on 100W MOPA Compensate for thermal lens in second slab by using cylindrical lenses in triple pass. Faster beam quality measurements using holographic beam sampler to eliminate need for multiple wedges for attenuating power. M 2 measurement of MOPA output. Redo theoretical calculation of thermal lens.

End pumping topology for 200W design Motivation -> Higher efficiency Near total absorption of pump light. Confinement of pump radiation leads to better mode overlap signal IN Pump 0.6% Nd:YAG undoped end signal OUT

Pre-amplifier Design : End-pumping 20 W 160 W 2-slab end-pumped double passed amplifier Crystal Dimensions Width = 1.11 mm, Length = 6.6 cm, Thickness = 0.9 mm Slab Design Issues 1. Parasitic suppression 2. Pump light coupling and absorption Courtesy, Hagop Injeyan, TRW

Expected MOPA System Performance AmplifierInput Power Multi-mode Output Output TEM 00 End-pumped (P pump = 130W) 16W60W48W End-pumped (P pump = 435W) 48W200W160W Edge-pumped (P pump = 1400W) 160W500W400W Edge pumped design chosen for final stage because of heat extraction requirement and simpler engineering design without sacrificing much pump absorption.

Status of 200W design Received 8mm x 8mm Nd:YAG composites with undoped ends from Onyx. Diced up one composite in the Stanford Crystal shop. On one plate undoped end broke off cleanly from the doped portion. (possibly defective bonding from Onyx?)

Status of 200W design (contd….) Second composite being diced up by Crystal River Optics.

Future Work on 200W MOPA Get coated plates from MLD, inspect and dice up into slabs with final dimensions. Install Laser Line pump diodes with total pump power of 500W. Fabricate laser head with microchannel coolers. Integrate and start amplifier experiments.