Testing post-Newtonian theory with gravitational wave observations
| 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.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.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.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 |