Generalized Couch-Torrence symmetry for rotating extremal black holes in maximal supergravity

Cvetič, M.; Pope, C. N.; Saha, A.

doi:10.1103/PhysRevD.102.086007

Title: Generalized Couch-Torrence symmetry for rotating extremal black holes in maximal supergravity

Journal Article · Thu Oct 08 00:00:00 EDT 2020 · Physical Review. D.

DOI:https://doi.org/10.1103/PhysRevD.102.086007· OSTI ID:1671155

Cvetič, M.; Pope, C. N.;

The extremal Reissner-Nordström black hole admits a conformal inversion symmetry, in which the metric is mapped into itself under an inversion of the radial coordinate combined with a conformal rescaling. In the rotating generalization, Couch and Torrence showed that the Kerr-Newman metric no longer exhibits a conformal inversion symmetry, but the radial equation arising in the separation of the massless Klein-Gordon equation admits a mode-dependent inversion symmetry, where the radius of inversion depends upon the energy and azimuthal angular momentum of the mode.

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Research Organization:: Univ. of Pennsylvania, Philadelphia, PA (United States); Texas A & M Univ., College Station, TX (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: SC0013528; FG02-13ER42020; SC0010813

OSTI ID:: 1671155

Alternate ID(s):: OSTI ID: 1684629

Journal Information:: Physical Review. D., Journal Name: Physical Review. D. Vol. 102 Journal Issue: 8; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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79 ASTRONOMY AND ASTROPHYSICS
Classical black holes
supergravity
supersymmetry
conformal symmetry

Title: Generalized Couch-Torrence symmetry for rotating extremal black holes in maximal supergravity

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