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Overspinning a Kerr black hole: The effect of the self-force

Overspinning a Kerr black hole: The effect of the self-force
Overspinning a Kerr black hole: The effect of the self-force
We study the scenario in which a massive particle is thrown into a rapidly rotating Kerr black hole in an attempt to spin it up beyond its extremal limit, challenging weak cosmic censorship. We work in black-hole perturbation theory, and focus on nonspinning, uncharged particles sent in on equatorial orbits. We first identify the complete parameter-space region in which overspinning occurs when backreaction effects from the particle’s self-gravity are ignored. We find, in particular, that overspinning can be achieved only with particles sent in from infinity. Gravitational self-force effects may prevent overspinning by radiating away a sufficient amount of the particle’s angular momentum (“dissipative effect”), and/or by increasing the effective centrifugal repulsion, so that particles with suitable parameters never get captured (“conservative effect”). We analyze the full effect of the self-force, thereby completing previous studies by Jacobson and Sotiriou (who neglected the self-force) and by Barausse, Cardoso and Khanna (who considered the dissipative effect on a subset of orbits). Our main result is an inequality, involving certain self-force quantities, which describes a necessary and sufficient condition for the overspinning scenario to be overruled. This “censorship” condition is formulated on a certain one-parameter family of geodesics in the limit of an extremal Kerr geometry. We find that the censorship condition is insensitive to the dissipative effect (within the first-order self-force approximation used here), except for a subset of perfectly fine-tuned orbits, for which a separate censorship condition is derived. We do not obtain here the self-force input needed to evaluate either of our two conditions, but discuss the prospects for producing the necessary data using state-of-the-art numerical codes.
1550-7998
Colleoni, Marta
8d640b05-0199-47d1-8bd5-8fafa5533fee
Barack, Leor
f08e66d4-c2f7-4f2f-91b8-f2c4230d0298
Colleoni, Marta
8d640b05-0199-47d1-8bd5-8fafa5533fee
Barack, Leor
f08e66d4-c2f7-4f2f-91b8-f2c4230d0298

Colleoni, Marta and Barack, Leor (2015) Overspinning a Kerr black hole: The effect of the self-force. Physical Review D, 91 (10), [104024]. (doi:10.1103/PhysRevD.91.104024).

Record type: Article

Abstract

We study the scenario in which a massive particle is thrown into a rapidly rotating Kerr black hole in an attempt to spin it up beyond its extremal limit, challenging weak cosmic censorship. We work in black-hole perturbation theory, and focus on nonspinning, uncharged particles sent in on equatorial orbits. We first identify the complete parameter-space region in which overspinning occurs when backreaction effects from the particle’s self-gravity are ignored. We find, in particular, that overspinning can be achieved only with particles sent in from infinity. Gravitational self-force effects may prevent overspinning by radiating away a sufficient amount of the particle’s angular momentum (“dissipative effect”), and/or by increasing the effective centrifugal repulsion, so that particles with suitable parameters never get captured (“conservative effect”). We analyze the full effect of the self-force, thereby completing previous studies by Jacobson and Sotiriou (who neglected the self-force) and by Barausse, Cardoso and Khanna (who considered the dissipative effect on a subset of orbits). Our main result is an inequality, involving certain self-force quantities, which describes a necessary and sufficient condition for the overspinning scenario to be overruled. This “censorship” condition is formulated on a certain one-parameter family of geodesics in the limit of an extremal Kerr geometry. We find that the censorship condition is insensitive to the dissipative effect (within the first-order self-force approximation used here), except for a subset of perfectly fine-tuned orbits, for which a separate censorship condition is derived. We do not obtain here the self-force input needed to evaluate either of our two conditions, but discuss the prospects for producing the necessary data using state-of-the-art numerical codes.

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More information

e-pub ahead of print date: 20 May 2015
Published date: 20 May 2015
Organisations: Applied Mathematics

Identifiers

Local EPrints ID: 410388
URI: http://eprints.soton.ac.uk/id/eprint/410388
ISSN: 1550-7998
PURE UUID: 4203d239-e99b-410d-baa1-575a204db98d
ORCID for Leor Barack: ORCID iD orcid.org/0000-0003-4742-9413

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Date deposited: 07 Jun 2017 16:31
Last modified: 16 Mar 2024 03:41

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Contributors

Author: Marta Colleoni
Author: Leor Barack ORCID iD

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