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Paper detail

Testing post-Newtonian theory with gravitational wave observations

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.

preprint2006arXivOpen access
K. G. ArunB. R. IyerM. S. S. QusailahB. S. Sathyaprakash
astro-phgr-qc
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K. G. ArunB. R. IyerM. S. S. QusailahB. S. Sathyaprakash

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