Scalar radiation emitted from a source rotating around a black hole
From MaRDI portal
Publication:4934998
DOI10.1088/0264-9381/17/1/303zbMath0939.83034arXivgr-qc/9901006OpenAlexW2168567247MaRDI QIDQ4934998
Luís C. B. Crispino, Atsushi Higuchi, George E. A. Matsas
Publication date: 30 January 2000
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/9901006
Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20) Gravitational waves (83C35)
Related Items (8)
The real solution to scalar field equation in 5D black string space ⋮ THE SCALAR FIELD IN EXTREME REISSNER–NORDSTRÖM–DE SITTER SPACE ⋮ THE REAL SCALAR FIELD EQUATION FOR NARIAI BLACK HOLE IN THE 5D SCHWARZSCHILD–DE SITTER BLACK STRING SPACE ⋮ Geodesic synchrotron radiation in black hole spacetimes: analytical investigation ⋮ The scalar field equation in Schwarzschild-de Sitter space ⋮ Scalar radiation emitted by a source around a spherically symmetric black hole ⋮ RADIATION AND POTENTIAL BARRIERS OF A 5D BLACK STRING SOLUTION ⋮ Real scalar field scattering around the extreme Reissner-Nordström black hole in de Sitter spacetime
This page was built for publication: Scalar radiation emitted from a source rotating around a black hole