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dc.contributor.authorGralla, Samuel E
dc.contributor.authorHughes, Scott A
dc.contributor.authorWarburton, Niels J
dc.date.accessioned2019-05-29T19:27:46Z
dc.date.available2019-05-29T19:27:46Z
dc.date.issued2016-07
dc.date.submitted2016-03
dc.identifier.issn0264-9381
dc.identifier.issn1361-6382
dc.identifier.urihttps://hdl.handle.net/1721.1/121177
dc.description.abstractWe model the inspiral of a compact object into a more massive black hole rotating very near the theoretical maximum. We find that once the body enters the near-horizon regime the gravitational radiation is characterized by a constant frequency, equal to (twice) the horizon frequency, with an exponentially damped profile. This contrasts with the usual 'chirping' behavior and, if detected, would constitute a 'smoking gun' for a near-extremal black hole in nature.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant PHY–1403261)en_US
dc.description.sponsorshipMarie Curie International Fellowship (Award PIOF-GA-2012-627781)en_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/0264-9381/33/15/155002en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourcearXiven_US
dc.titleInspiral into Gargantuaen_US
dc.typeArticleen_US
dc.identifier.citationGralla, Samuel E et al. “Inspiral into Gargantua.” Classical and Quantum Gravity 33, 15 (July 2016): 155002 © 2016 IOP Publishing Ltden_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.relation.journalClassical and Quantum Gravityen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2019-03-26T17:33:57Z
dspace.orderedauthorsGralla, Samuel E; Hughes, Scott A; Warburton, Nielsen_US
dspace.embargo.termsNen_US
dspace.date.submission2019-04-04T11:53:30Z
mit.licenseOPEN_ACCESS_POLICYen_US
mit.licenseOPEN_ACCESS_POLICY


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