'Tem 00' diaporamas de présentation

Development of high-power and stable laser for gravitational wave detection

Development of high-power and stable laser for gravitational wave detection. Mio Laboratory Kohei Takeno. Aims of My Work. Current Status. Final Goal. Nd:YAG ? 1.064 m m ? Output Power ? 100W Single Transverse Mode Single Longitudinal Mode Low Intensity Noise Low Frequency Noise

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Design of an Output Mode Cleaner to Enable DC Readout in the LIGO 40-Meter Interferometer

Design of an Output Mode Cleaner to Enable DC Readout in the LIGO 40-Meter Interferometer. Marcus Ng Mentor: Alan Weinstein Co-mentor: Robert Ward. Overview. LIGO 40m Gaussian beams OMC design criteria OMC Parameters Geometry Guoy Phase ROC g-factor Finesse Mirror Transmission

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Experimental test of higher-order LG modes in the 10m Glasgow prototype interferometer

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Status of high power laser development for LIGO at Stanford

Status of high power laser development for LIGO at Stanford. Shally Saraf*, Supriyo Sinha, Arun Kumar Sridharan and Robert L. Byer E. L. Ginzton Laboratory, Stanford University. LSC2003 Hannover, Germany August 18-21, 2003. LIGO-G030434-00-Z. * saraf@stanford.edu. Outline.

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Ultra-stable, high-power laser systems

Ultra-stable, high-power laser systems. Patrick Kwee on behalf of AEI Hannover and LZH Advanced detectors session, 26. March 2011. Albert-Einstein-Institut Hannover. Motivation. Laser noise couples to GW read out channel. Reduce coupling Null instrument, ...

353 views • 17 slides

Motivation: Physical Conditions in LHDAC experiments. Exploration of parameter space:

Finite-Element Modeling of the Thermal Structure in Laser-Heated Diamond Anvil Cell Experiments. Boris Kiefer Physics Department; New Mexico State University, NM, USA. Tom. S. Duffy Department of Geosciences, Princeton University, Princeton, USA. Motivation: Physical Conditions in LHDAC

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Studies of Thermal Loading in Pre-Modecleaners for Advanced LIGO

Studies of Thermal Loading in Pre-Modecleaners for Advanced LIGO. Amber Bullington Stanford University LSC/Virgo March 2007 Meeting Optics Working Group G070084-00-Z. Outline. Thermal Loading Experiment Ring cavity known as pre-modecleaner (PMC) Same geometry as cavity used in the PSL

249 views • 12 slides