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dc.contributor.authorYunes, Nicolas
dc.contributor.authorKocsis, Bence
dc.contributor.authorLoeb, Abraham
dc.contributor.authorHaiman, Zoltan
dc.date.accessioned2012-02-09T18:38:32Z
dc.date.available2012-02-09T18:38:32Z
dc.date.issued2011-10
dc.date.submitted2011-03
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.urihttp://hdl.handle.net/1721.1/69068
dc.description.abstractWe study the effects of a thin gaseous accretion disk on the inspiral of a stellar-mass black hole into a supermassive black hole. We construct a phenomenological angular momentum transport equation that reproduces known disk effects. Disk torques modify the gravitational wave phase evolution to detectable levels with LISA for reasonable disk parameters. The Fourier transform of disk-modified waveforms acquires a correction with a different frequency trend than post-Newtonian vacuum terms. Such inspirals could be used to detect accretion disks with LISA and to probe their physical parameters.en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration. Einstein Postdoctoral Fellowship Award (PF9-00063)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration. Einstein Postdoctoral Fellowship Award (PF0-110080)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (NAS8-03060)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (grant AST-0907890)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (grant NNX08AL43G)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (grant NNA09DB30A)en_US
dc.description.sponsorshipNational Office for Research and Technology (Hungary) (Polanyi Program)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (grant NNX08AH35G)en_US
dc.description.sponsorshipHungarian Scientific Research Foundation (OTKA) (grant 68228)en_US
dc.language.isoen_US
dc.publisherAmerican Physical Society (APS)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevLett.107.171103en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAPSen_US
dc.titleImprint of Accretion Disk-Induced Migration on Gravitational Waves from Extreme Mass Ratio Inspiralsen_US
dc.typeArticleen_US
dc.identifier.citationYunes, Nicolás et al. “Imprint of Accretion Disk-Induced Migration on Gravitational Waves from Extreme Mass Ratio Inspirals.” Physical Review Letters 107.17 (2011): n. pag. Web. 9 Feb. 2012. © 2011 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.approverYunes, Nicolas
dc.contributor.mitauthorYunes, Nicolas
dc.relation.journalPhysical Review Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsYunes, Nicolás; Kocsis, Bence; Loeb, Abraham; Haiman, Zoltánen
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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