Inspiral into Gargantua.

Bibliographic Details
Title: Inspiral into Gargantua.
Authors: Samuel E Gralla1,2, Scott A Hughes3,4, Niels Warburton4,5 nielsw@mit.edu
Source: Classical & Quantum Gravity. 8/4/2016, Vol. 33 Issue 15, p1-1. 1p.
Subject Terms: *BLACK holes, *GRAVITATIONAL waves, *COMPACT objects (Astronomy), *GRAVITATIONAL collapse, *GRAVITATIONAL fields
Abstract: We 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. [ABSTRACT FROM AUTHOR]
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  Data: <searchLink fieldCode="AR" term="%22Samuel+E+Gralla%22">Samuel E Gralla</searchLink><relatesTo>1,2</relatesTo><br /><searchLink fieldCode="AR" term="%22Scott+A+Hughes%22">Scott A Hughes</searchLink><relatesTo>3,4</relatesTo><br /><searchLink fieldCode="AR" term="%22Niels+Warburton%22">Niels Warburton</searchLink><relatesTo>4,5</relatesTo><i> nielsw@mit.edu</i>
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  Data: *<searchLink fieldCode="DE" term="%22BLACK+holes%22">BLACK holes</searchLink><br />*<searchLink fieldCode="DE" term="%22GRAVITATIONAL+waves%22">GRAVITATIONAL waves</searchLink><br />*<searchLink fieldCode="DE" term="%22COMPACT+objects+%28Astronomy%29%22">COMPACT objects (Astronomy)</searchLink><br />*<searchLink fieldCode="DE" term="%22GRAVITATIONAL+collapse%22">GRAVITATIONAL collapse</searchLink><br />*<searchLink fieldCode="DE" term="%22GRAVITATIONAL+fields%22">GRAVITATIONAL fields</searchLink>
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  Data: We 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. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of Classical & Quantum Gravity is the property of IOP Publishing and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1088/0264-9381/33/15/155002
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        Type: general
      – SubjectFull: GRAVITATIONAL waves
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      – SubjectFull: GRAVITATIONAL collapse
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      – SubjectFull: GRAVITATIONAL fields
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      – TitleFull: Inspiral into Gargantua.
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              Text: 8/4/2016
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