Gravitational wave astronomy: Recent advances

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2830

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DC Field	Value	Language
dc.contributor.author	Dhurandhar, S. V	-
dc.date.accessioned	2008-07-23T07:04:22Z	-
dc.date.available	2008-07-23T07:04:22Z	-
dc.date.issued	2002-09	-
dc.identifier.citation	BASI, Vol. 30, No. 3, pp. 729 - 734	en
dc.identifier.uri	http://hdl.handle.net/2248/2830	-
dc.description.abstract	Several groundbased gravitational wave (GW) laser interferometric projects have completed construction and are currently involved in conducting engineering runs. The spacebased NASA-ESA mission, LISA is expected to be launched in ten years' time. With the data around the comer exciting times lie ahead for GW astronomy. A brief introduction to GW detection, the principle of GW detection, the current status of ground based detectors, the space based detector LISA, GW sources and the data analysis necessary to extract the weak GW signal from the detector noise will be presented.	en
dc.format.extent	251576 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Gravitational Waves	en
dc.subject	Interferometric Detectors	en
dc.subject	Astrophysical GW Sources	en
dc.title	Gravitational wave astronomy: Recent advances	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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