Gravitational Wave Detection – current status & future prospects. Jonathan Gair. Extragalactic Group Seminar, IoA, 21 st November 2005. Gravitational Waves. Fluctuations in spacetime curvature, generated by rapidly accelerating masses.By derex
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GEO-LIGO data analysis. M.Alessandra Papa Max Planck Inst. f. Gravitationsphysik, Potsdam, Germany G040534-00-Z VESF foundation meeting, Pisa, Dec. 2004. data analysis experiment. GEO 600 Project. Albert Einstein Institute (Golm and Hannover) University of the Balearic Islands
What is LIGO (LSC/GEO/Virgo/…)?. Virgo detector, Cascina , Italy. Gabriela Gonz ález , Louisiana State University For the LIGO Scientific Collaboration and the Virgo Collaboration. LIGO Hanford Observatory Washington, USA. LIGO Livingston Observatory, Louisiana, USA.
The GEO 600 Laser System LIGO-G010366-00-Z. V. Quetschke°, M. Kirchner°, I .Zawischa*, M. Brendel*, C. Fallnich*, S. Nagano + , B. Willke° + , K. Danzmann° + , and the GEO600 Team *Laser Zentrum Hannover, Hollerithallee 8, D-30419 Hannover, Germany
Searching for Gravitational Waves with LIGO, GEO and Einstein@home. Michael Landry LIGO Hanford Observatory California Institute of Technology. "Colliding Black Holes" Credit: National Center for Supercomputing Applications (NCSA). Here’s what we’ll go through. What are gravitational waves?
LIGO. Outreach. Southern University – LIGO Educational Outreach Collaboration: An Overview S. C. McGuire Department of Physics Southern University and A&M College Baton Rouge, LA 70813 * Work supported by NSF Grants No. PHY-0101177 and PHY-0355471.
LIGO Overview. Barry Barish PAC - LLO 5-Dec-02. LIGO schedule and plan. Primary Activities. 1996 Construction Underway (mostly civil) 1997 Facility Construction (vacuum system) 1998 Interferometer Construction (complete facilities)
Advanced LIGO. David Shoemaker Aspen at Elba 23 May 2002. Core notions for the LIGO Lab future. Evolution intrinsic to LIGO mission: to enable the development of gravitational wave astronomy Next step in detector design:
Advanced LIGO. David Shoemaker Aspen 3 February 03. Advanced LIGO. LIGO mission: detect gravitational waves and initiate GW astronomy Next detector Must be of significance for astrophysics Should be at the limits of reasonable extrapolations of detector physics and technologies
Advanced LIGO. David Shoemaker NSF Review of Advanced LIGO 11 June 2003. Advanced LIGO. LIGO mission: detect gravitational waves and initiate GW astronomy Next detector Must be of significance for astrophysics
Einstein's Legacy: General Relativity, our Best Description of the Universe Barry C. Barish Caltech AAAS 20-Feb-05. Crab Pulsar. LIGO-xxx. General Relativity the essential idea. G mn = 8 pT mn. Gravity is not a force, but a property of space & time Spacetime = 3 spatial dimensions + time