期刊
CLASSICAL AND QUANTUM GRAVITY
卷 22, 期 10, 页码 S375-S379出版社
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/22/10/032
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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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