Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2831
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dc.contributor.authorIyer, B. R-
dc.date.accessioned2008-07-23T07:10:27Z-
dc.date.available2008-07-23T07:10:27Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 735 - 740en
dc.identifier.urihttp://hdl.handle.net/2248/2831-
dc.description.abstractKilometer scale Laser Interferometer Gravitational Wave Detectors like LIGO (vntGO) are expected to go online in 2002 (2003). Space interferometers like LISA are scheduled for 2011. In this talk the possible science payoffs of these experiments are explored. Starting from the basic properties of gravitational waves and anticipated gravitational wave sources, it highlights the implications of gravitational wave observations for basic physics, astrophysics and cosmology. The current status of theoretical computation of waveforms and templates for data analysis is briefly discussed.en
dc.format.extent252234 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectLIGOen
dc.subjectVIRGOen
dc.subjectGravitational Wave Astronomyen
dc.titleGravitational Wave Astronomy:Probing Physics and Unravelling Astrophysicsen
dc.typeArticleen
Appears in Collections:BASI Publications

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