Testing post-Newtonian theory with gravitational wave observations

K. G. Arun, B. R. Iyer, M. S.S. Qusailah, B. S. Sathyaprakash

Research output: Contribution to journalArticle

56 Citations (Scopus)

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.

Original languageEnglish (US)
Pages (from-to)L37-L43
JournalClassical and Quantum Gravity
Volume23
Issue number9
DOIs
StatePublished - May 7 2006

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gravitational waves
antennas
lasers
relativity
signal to noise ratios
gravitation
probes

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy (miscellaneous)

Cite this

Arun, K. G. ; Iyer, B. R. ; Qusailah, M. S.S. ; Sathyaprakash, B. S. / Testing post-Newtonian theory with gravitational wave observations. In: Classical and Quantum Gravity. 2006 ; Vol. 23, No. 9. pp. L37-L43.
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Testing post-Newtonian theory with gravitational wave observations. / Arun, K. G.; Iyer, B. R.; Qusailah, M. S.S.; Sathyaprakash, B. S.

In: Classical and Quantum Gravity, Vol. 23, No. 9, 07.05.2006, p. L37-L43.

Research output: Contribution to journalArticle

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