An axionic Kerr black hole
- 1 August 1991
- journal article
- Published by IOP Publishing in Classical and Quantum Gravity
- Vol. 8 (8) , L161-L165
- https://doi.org/10.1088/0264-9381/8/8/002
Abstract
An axionic Kerr black hole solution, which has Kerr-like metric and non-vanishing axionic field strength, has been found exactly by solving the stationary axisymmetric Einstein axion field equation. It indicates that there exists an axionic hair for the rotating black hole and the axionic hair can be detected by strings directly, without resorting to the Aharonov-Bohm process. In addition, some interesting characteristics for the structure of an axionic Kerr black hole are also studied.Keywords
This publication has 12 references indexed in Scilit:
- Axion hair for Kerr black holesPublished by Elsevier ,2002
- A proof of the uniqueness theorem for axionic black holesClassical and Quantum Gravity, 1991
- Axionic black holes and wormholesGeneral Relativity and Gravitation, 1990
- Effective Lagrangians for the string model of Bluhm, Dolan, and Goddard. II. The fermionic sectorPhysical Review D, 1989
- Effective Lagrangians for the string model of Bluhm, Dolan, and Goddard. I. The bosonic sectorPhysical Review D, 1989
- Axionic Black Holes and an Aharonov-Bohm Effect for StringsPhysical Review Letters, 1988
- Four-dimensional heterotic strings and conformal field theoryNuclear Physics B, 1988
- Four-dimensional supergravity from four-dimensional stringsNuclear Physics B, 1988
- The quartic effective action for the heterotic stringNuclear Physics B, 1987
- Birkhoff's theorem for general Riemann-Cartan-typetheories of gravityPhysical Review D, 1981