Interaction of Hawking radiation with static sources outside a Schwarzschild black hole

Atsushi Higuchi, George E. A. Matsas, and Daniel Sudarsky
Phys. Rev. D 58, 104021 – Published 22 October 1998
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Abstract

We show that the response rate of (i) a static source interacting with Hawking radiation of a massless scalar field in Schwarzschild spacetime (with the Unruh vacuum) and that of (ii) a uniformly accelerated source with the same proper acceleration in Minkowski spacetime (with the Minkowski vacuum) are equal. We show that this equality will not hold if the Unruh vacuum is replaced by the Hartle-Hawking vacuum. It is verified that the source responds to the Hawking radiation near the horizon as if it were at rest in a thermal bath in Minkowski spacetime with the same temperature. It is also verified that the response rate in the Hartle-Hawking vacuum approaches that in Minkowski spacetime with the same temperature far away from the black hole. Finally, we compare our results with others in the literature.

  • Received 16 June 1998

DOI:https://doi.org/10.1103/PhysRevD.58.104021

©1998 American Physical Society

Authors & Affiliations

Atsushi Higuchi

  • Institut für theoretische Physik, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland
  • Department of Mathematics, University of York, Heslington, York YO10 5DD, United Kingdom

George E. A. Matsas

  • Instituto de Física Teórica, Universidade Estadual Paulista, Rua Pamplona 145, 01405-900–São Paulo, São Paulo, Brazil

Daniel Sudarsky

  • Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, A. Postal 70/543, Mexico D.F. 04510, Mexico

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Vol. 58, Iss. 10 — 15 November 1998

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