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LIGO SCIENCE

LIGO SCIENCE. Kip S. Thorne CaRT, California Institute of Technology LIGO PAC Meeting Pasadena, 5 June 2003 LIGO-G030293-00-R. 300 in h ~10 7 in rate. Most Optimistic Source Strengths. h rms = h(f) ?f ~ 10 h(f). Open up wider band. 15 in h ~3000 in rate. Most Pessimistic

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350 views • 20 slides

ASTROPHYSICS

ASTROPHYSICS. Kip S. Thorne CaRT, California Institute of Technology NSF Advanced LIGO Review Pasadena, 11 June 2003. 300 in h ~10 7 in rate. Most Optimistic Source Strengths. h rms = h(f) ?f ~ 10 h(f). Open up wider band. 15 in h ~3000 in rate. Most Pessimistic

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330 views • 20 slides

LIGO SCIENCE

LIGO SCIENCE. Kip S. Thorne CaRT, California Institute of Technology NSF LIGO Operations Panel Hanford - 26 February 2001. LIGO-G010183-00-M. 300 in h ~10 7 in rate. Most Optimistic Source Strengths. h rms = h(f) ?f ~ 10 h(f). Open up wider band. 15 in h ~3000 in rate.

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292 views • 18 slides

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LIGO SCIENCE

ASTROPHYSICS

LIGO SCIENCE