Black-hole evaporation in the Klein-Sauter-Heisenberg-Euler formalism
- 15 July 1976
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 14 (2) , 332-334
- https://doi.org/10.1103/physrevd.14.332
Abstract
A generalization of the classical approach of barrier penetration introduced by Klein, Sauter, Heisenberg, and Euler to curved spaces endowed with future horizons is given. This technique allows one to recover most directly results obtained by Hawking recently. The treatment here presented encompasses, as special cases, the works of Deruelle and Ruffini, of Damour and Ruffini, and of Nakamura and Sato.Keywords
This publication has 16 references indexed in Scilit:
- Quantum Electrodynamical Effects in Kerr-Newmann GeometriesPhysical Review Letters, 1975
- Klein paradox in a kerr geometryPhysics Letters B, 1975
- Second quantization in the Kerr metricPhysical Review D, 1974
- Quantum and classical relativistic energy states in stationary geometriesPhysics Letters B, 1974
- On the generalized ergosphere of the Kerr-Newman geometryPhysics Letters B, 1974
- Upper bound on the electric charge of a black holeNature, 1974
- On the energetics of Reissner Nordstrøm geometriesPhysics Letters B, 1973
- Reversible Transformations of a Charged Black HolePhysical Review D, 1971
- Gravitational Radiation from Colliding Black HolesPhysical Review Letters, 1971
- Reversible and Irreversible Transformations in Black-Hole PhysicsPhysical Review Letters, 1970