Search for gravitational wave ringdowns from perturbed black holes in LIGO S4 data

Search for gravitational wave ringdowns from perturbed black holes in LIGO S4 data

According to general relativity a perturbed black hole will settle to a stationary configuration by the emission of gravitational radiation. Such a perturbation will occur, for example, in the coalescence of a black hole binary, following their inspiral and subsequent merger. At late times the wavef...

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Bibliographic Details
Main Authors: Wipf, Christopher C., Weiss, Rainer, Waldman, Samuel J., Stein, Leo Chaim, Stein, Andrew J., Smith, Nicolas de Mateo, Shapiro, B., Sarin, P., Markowitz, Jared John, Katsavounidis, Erotokritos, Hughey, Brennan J., Harry, Gregory, Grimaldi, F., Goda, K., Foley, Stephany, Duke, I., Cao, Junwei, Brunet, G., Blackburn, Lindy L., Barsotti, Lisa, Mavalvala, Nergis, Donovan, Frederick J, Corbitt, Thomas R, Bodiya, Timothy P., Zucker, Michael E, Shoemaker, David H, Ruet, Laurent, Mittleman, Richard K, Mason, Kenneth R, MacInnis, Myron E, Fritschel, Peter K, Evans, Matthew J
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: American Physical Society 2010
Online Access:http://hdl.handle.net/1721.1/52012
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0001-6550-3045
https://orcid.org/0000-0002-4147-2560
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0002-2544-1596
https://orcid.org/0000-0003-1983-3187

Internet

http://hdl.handle.net/1721.1/52012
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0001-6550-3045
https://orcid.org/0000-0002-4147-2560
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0002-2544-1596
https://orcid.org/0000-0003-1983-3187

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