Rotating black hole in asymptotic de Sitter space: Perturbation of the space-time with spin fields

Journal Article · Thu Sep 15 04:00:00 EDT 1983 · Phys. Rev. D; (United States)

DOI:https://doi.org/10.1103/PhysRevD.28.1291· OSTI ID:5812571

Khanal, U

The Newman-Penrose formalism is used to work with gravitational, electromagnetic, and Dirac field perturbations of the Kerr--de Sitter space. It is shown that the resulting equations are separable, and the radial parts (for the massless fields) combine into a master equation resembling that of Teukolsky. This master equation includes the Teukolsky equation and the equation arising from the de Sitter--Schwarzschild universe, and can be reduced to these cases under appropriate limiting conditions. Finally, the radial parts of the electromagnetic and neutrino fields are transformed to the form of the one-dimensional barrier-penetration equation.

• Research Organization: Department of Physics, Tribhuvan University, Kirtipur, Nepal
• OSTI ID: 5812571
• Journal Information: Phys. Rev. D; (United States), Journal Name: Phys. Rev. D; (United States) Vol. 28:6; ISSN PRVDA
• Country of Publication: United States
• Language: English

Related Subjects

640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
640106 -- Astrophysics & Cosmology-- Cosmology
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANGULAR MOMENTUM
BLACK HOLES
COSMOLOGY
DIRAC COSMOLOGY
ELEMENTARY PARTICLES
FERMIONS
GRAVITATIONAL FIELDS
LEPTONS
MASSLESS PARTICLES
MOTION
NEUTRINOS
PARTICLE PROPERTIES
PERTURBATION THEORY
ROTATION
SPACE-TIME
SPIN
UNIVERSE