Extreme mass ratio binary radiation reaction and gravitational waveform
Identifieur interne : 000303 ( Main/Exploration ); précédent : 000302; suivant : 000304Extreme mass ratio binary radiation reaction and gravitational waveform
Auteurs : Yasushi Mino [États-Unis]Source :
- Classical and Quantum Gravity [ 0264-9381 ] ; 2005.
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 recent theoretical progress in calculating the waveforms from such a system.
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DOI: 10.1088/0264-9381/22/10/032
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