Published October 7, 2006
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Search for black hole ringdown signals in LIGO S4 data
Abstract
If a coalescing binary system results in a black hole we expect it to be a perturbed Kerr black hole and to radiate gravitational waves in the form of ringdowns. A search for such signals in data from the fourth LIGO science run is currently being developed. In this paper we outline the theory on which this search is based and use it to predict the range for this data set.
Additional Information
© 2006 IOP Publishing Limited Received 31 March 2006, in final form 14 June 2006; Published 15 September 2006; Print publication: Issue 19 (7 October 2006) The author gratefully acknowledges the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max Planck Society and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The author also gratefully acknowledges the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educación y Ciencia, the John Simon Guggenheim Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation and the Alfred P Sloan Foundation.Files
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- Eprint ID
- 5496
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- CaltechAUTHORS:GOGcqg06
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2006-10-20Created from EPrint's datestamp field
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2022-07-12Created from EPrint's last_modified field