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Gravitational Wave Detection – current status & future prospects

Gravitational Wave Detection – current status & future prospects

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.

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Advanced LIGO

Advanced LIGO

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:

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Advanced LIGO

Advanced LIGO

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

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Advanced LIGO

Advanced LIGO

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

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Advanced LIGO

Advanced LIGO

Advanced LIGO. David Ottaway, for the LIGO Scientific Collaboration Aspen Winter Conference Feb 2004. Advanced LIGO. LIGO mission: detect gravitational waves and initiate GW astronomy Next detector Should have assured detectability of known sources

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Advanced LIGO

Advanced LIGO

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:

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Advanced LIGO

Advanced LIGO

Advanced LIGO. 5 July 2012. David Shoemaker For the LIGO Scientific Collaboration. Advanced LIGO. Goal: open the era of gravitational-wave astronomy through the direct detection of gravitational waves. Replaces the instruments at the Washington and Louisiana sites

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Advanced LIGO

Advanced LIGO

Advanced LIGO. Detector upgrade is planned for 2011-2014 Factor of 10 increase in distance probed (‘reach’) Factor of 1000 increase in event rate Fabrication began in 2009 Long lead time parts Mirror blanks, polishing, coating. The LIGO Detector. Advanced LIGO. 125 W laser

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Advanced LIGO

Advanced LIGO

Advanced LIGO. Dennis Coyne David Shoemaker Hannover LSC 19 August 2003. Advanced LIGO. Advanced LIGO proposal submitted, February 2003 3 interferometers, each 4km Signal recycled configuration ~180 W laser Sapphire substrates Quad monolithic suspensions Active isolation system

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Advanced LIGO

Advanced LIGO

Advanced LIGO. David Shoemaker AAAS Conference 17 February 2003. The LIGO Mission. LIGO Observatory Infrastructure in place Designed to support the evolving field of gravitational wave science Initial LIGO in operation Sensitivity improving steadily, approaching goal

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Advanced LIGO

Advanced LIGO

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 Should have assured detectability of known sources

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