Renormalized electromagnetic stress tensor in Schwarzschild spacetime

B. P. Jensen and Adrian Ottewill
Phys. Rev. D 39, 1130 – Published 15 February 1989
PDFExport Citation
Abstract
Authors
References

Abstract

The renormalized quantum stress tensor for an electromagnetic field in the Hartle-Hawking state in Schwarzschild spacetime is calculated using a mode sum which is evaluated numerically. The results shed light on stress-tensor-approximation methods that have been proposed in recent years.

  • Received 23 August 1988

DOI:https://doi.org/10.1103/PhysRevD.39.1130

©1989 American Physical Society

Authors & Affiliations

B. P. Jensen

  • Groupe d’Astrophysique Relativiste-CNRS, DARC, Observatoire de Paris, section de Meudon, 92195 Meudon Principal CEDEX, France
  • Institut für Theoretische Physik, Universität Bern, Sidlerstrasse 5, 3012 Bern, Switzerland

Adrian Ottewill

  • Groupe d’Astrophysique Relativiste-CNRS, DARC, Observatoire de Paris, section de Meudon, 92195 Meudon Principal CEDEX, France
  • Mathematical Institute, Oxford University, 24-29 St. Giles, Oxford OX1 3LB, England

References (Subscription Required)

Click to Expand
Issue

Vol. 39, Iss. 4 — 15 February 1989

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

Authorization Required

Log In
Other Options
×

Download & Share

PDFExportReuse & PermissionsCiting Articles (69)
×

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
×