Extreme Mass Ratio Binary: Radiation reaction and gravitational waveform
arXiv:gr-qc/0506008 · doi:10.1088/0264-9381/22/10/032
Abstract
For a successful detection of gravitational waves by LISA, it is essential to construct theoretical waveforms in a reliable manner. We discuss gravitational waves from an extreme mass ratio binary system which is expected to be a promising target of the LISA project. The extreme mass ratio binary is a binary system of a supermassive black hole and a stellar mass compact object. As the supermassive black hole dominates the gravitational field of the system, we suppose that the system might be well approximated by a metric perturbation of a Kerr black hole. We discuss a recent theoretical progress in calculating the waveforms from such a system.
Classical and Quantum Gravity 22 (2005) S375-S379, Proceedings for 5th International LISA Symposium
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