Perturbations of charged black holes

Journal Article · Sat May 15 04:00:00 EDT 1976 · Phys. Rev., D; (United States)

DOI:https://doi.org/10.1103/PhysRevD.13.2713· OSTI ID:7285267

Chitre, D M

Wave equations are derived in the Newman--Penrose formalism for gravitational and electromagnetic perturbations produced by charged and uncharged matter moving in a Reissner--Nordstrom background geometry. A brief sketch is given to obtain similar sets of equations in the Kerr--Newman background. The wave equations in the Kerr--Newman background, however, do not seem to separate, at least for the variables and the coordinate system used here. (AIP)

• Research Organization: Department of Physics, University of California, Santa Barbara, California 93106
• OSTI ID: 7285267
• Journal Information: Phys. Rev., D; (United States), Journal Name: Phys. Rev., D; (United States) Vol. 13:10; ISSN PRVDA
• Country of Publication: United States
• Language: English

Related Subjects

640102 -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
657003* -- Theoretical & Mathematical Physics-- Relativity & Gravitation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BASIC INTERACTIONS
BLACK HOLES
DISTURBANCES
ELECTROMAGNETIC INTERACTIONS
GAUGE INVARIANCE
GRAVITATIONAL COLLAPSE
GRAVITATIONAL FIELDS
GRAVITATIONAL INTERACTIONS
INTERACTIONS
INVARIANCE PRINCIPLES
KERR FIELD