Published May 21, 2005
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Journal Article
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Extreme mass ratio binary: radiation reaction and gravitational waveform
- Creators
- Mino, Yasushi
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.
Additional Information
© 2005 IOP Publishing Ltd. Received 19 October 2004, in final form 17 December 2004. Published 26 April 2005. Print publication: Issue 10 (21 May 2005) YM thanks Professor Kip Thorne and Professor Sterl Phinney for encouragement. YM was supported by NASA grant NAG5-12834 and NASA-ATP grant NNG04GK98G at CalTech.Files
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Additional details
- Eprint ID
- 582
- Resolver ID
- CaltechAUTHORS:MINcqg05
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2005-08-29Created from EPrint's datestamp field
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2022-07-12Created from EPrint's last_modified field