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 language||English (US)|
|Journal||Classical and Quantum Gravity|
|State||Published - May 7 2006|
All Science Journal Classification (ASJC) codes
- Physics and Astronomy (miscellaneous)