Black-hole evaporation in the Klein-Sauter-Heisenberg-Euler formalism

Thibaut Damour and Remo Ruffini
Phys. Rev. D 14, 332 – Published 15 July 1976
PDFExport Citation

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.

  • Received 3 November 1975

DOI:https://doi.org/10.1103/PhysRevD.14.332

©1976 American Physical Society

Authors & Affiliations

Thibaut Damour* and Remo Ruffini

  • Joseph Henry Physical Laboratories, Princeton, New Jersey 08540
  • Physics Department, University of Western Australia, Nedlands, Australia

  • *E. S. A. International fellow.
  • Alfred P. Sloan fellow.

Comments & Replies

Comment on the Damour-Ruffini treatment of black-hole evaporation

M. Martellini and A. Treves
Phys. Rev. D 15, 2415 (1977)

References (Subscription Required)

Click to Expand
Issue

Vol. 14, Iss. 2 — 15 July 1976

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×