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• W2077120151 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." @default.
• W2077120151 created "2016-06-24" @default.
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• W2077120151 date "2005-04-26" @default.
• W2077120151 modified "2023-10-17" @default.
• W2077120151 title "Extreme mass ratio binary: radiation reaction and gravitational waveform" @default.
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• W2077120151 doi "https://doi.org/10.1088/0264-9381/22/10/032" @default.
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