Testing post-Newtonian theory with gravitational wave observations
K. G. Arun, B. R. Iyer, M. S. S. Qusailah, B. S. Sathyaprakash
Abstract
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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