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arxiv: gr-qc/0604018 · v1 · pith:GLFDEX46new · submitted 2006-04-05 · 🌀 gr-qc · astro-ph

Testing post-Newtonian theory with gravitational wave observations

K.G. Arun , B.R. Iyer , M.S.S. Qusailah , B.S. Sathyaprakash This is my paper
classification 🌀 gr-qc astro-ph
keywords lisaobservationspost-newtoniantheoryaffordalternativesamplitudeantenna
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The Laser Interferometric Space Antenna (LISA) will observe supermassive black hole binary mergers with amplitude signal-to-noise ratio of several thousands. 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 non-linear structure of post-Newtonian theory both in the context of general relativity and its alternatives.

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