Author ORCID Identifier

0000-0002-1606-8208

Document Type

Article

Rights

Available under a Creative Commons Attribution Non-Commercial Share Alike 4.0 International Licence

Disciplines

1.1 MATHEMATICS, Applied mathematics, Particles and fields physics

Publication Details

Physical Review D 106, 065023

https://journals.aps.org/prd/abstract/10.1103/PhysRevD.106.065023

Abstract

In this paper, we describe an extremely efficient method for computing the renormalized stress-energy tensor of a quantum scalar field in spherically symmetric black hole spacetimes. The method applies to a scalar field with arbitrary field parameters. We demonstrate the utility of the method by computing the renormalized stress-energy tensor for a scalar field in the Schwarzschild black hole spacetime, applying our results to discuss the null energy condition and the semiclassical backreaction.

DOI

https://doi.org/10.1103/PhysRevD.106.065023


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