Testing post-Newtonian theory with gravitational wave observations

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1744

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DC Field	Value	Language
dc.contributor.author	Arun, K.G.	-
dc.contributor.author	Iyer, B.R.	-
dc.contributor.author	Qusailah, M.S.S.	-
dc.contributor.author	Sathyaprakash, B.S.	-
dc.date.accessioned	2007-01-08T05:47:31Z	-
dc.date.available	2007-01-08T05:47:31Z	-
dc.date.issued	2006-05-09	-
dc.identifier.citation	Classical and Quantum Gravity, 2006, Vol.23 pL37-L43	en
dc.identifier.issn	0264-9381	-
dc.identifier.issn	1361-6382 (Online)	-
dc.identifier.uri	http://hdl.handle.net/2289/1744	-
dc.description	Restricted Access. An open access version is available at arXiv.org.(one of the alternative locations)	en
dc.description.abstract	The Laser Interferometric Space Antenna (LISA) will observe supermassive black hole binary mergers with an amplitude signal-to-noise ratio of several thousand. We investigate the extent to which such observations afford high-precision tests of Einstein's gravity. We show that LISA provides a unique opportunity to probe the nonlinear structure of post-Newtonian theory both in the context of general relativity and its alternatives.	en
dc.format.extent	335097 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The IOP Publishing Ltd.	en
dc.relation.uri	http://dx.doi.org/10.1088/0264-9381/23/9/L01	en
dc.relation.uri	http://arxiv.org/abs/gr-qc/0604018	en
dc.rights	(2006) by the IOP Publishing Ltd.	en
dc.title	Testing post-Newtonian theory with gravitational wave observations	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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