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

Abstract

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.

Authors:
; ; ORCiD logo
Publication Date:
Research Org.:
Univ. of Pennsylvania, Philadelphia, PA (United States); Texas A & M Univ., College Station, TX (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1671155
Alternate Identifier(s):
OSTI ID: 1684629
Grant/Contract Number:  
SC0013528; FG02-13ER42020; SC0010813
Resource Type:
Journal Article: Published Article
Journal Name:
Physical Review D
Additional Journal Information:
Journal Name: Physical Review D Journal Volume: 102 Journal Issue: 8; Journal ID: ISSN 2470-0010
Publisher:
American Physical Society
Country of Publication:
United States
Language:
English

Citation Formats

Cvetič, M., Pope, C. N., and Saha, A. Generalized Couch-Torrence symmetry for rotating extremal black holes in maximal supergravity. United States: N. p., 2020. Web. doi:10.1103/PhysRevD.102.086007.
Cvetič, M., Pope, C. N., & Saha, A. Generalized Couch-Torrence symmetry for rotating extremal black holes in maximal supergravity. United States. doi:10.1103/PhysRevD.102.086007.
Cvetič, M., Pope, C. N., and Saha, A. Thu . "Generalized Couch-Torrence symmetry for rotating extremal black holes in maximal supergravity". United States. doi:10.1103/PhysRevD.102.086007.
@article{osti_1671155,
title = {Generalized Couch-Torrence symmetry for rotating extremal black holes in maximal supergravity},
author = {Cvetič, M. and Pope, C. N. and Saha, A.},
abstractNote = {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.},
doi = {10.1103/PhysRevD.102.086007},
journal = {Physical Review D},
issn = {2470-0010},
number = 8,
volume = 102,
place = {United States},
year = {2020},
month = {10}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record at 10.1103/PhysRevD.102.086007

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Works referenced in this record:

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