Hadamard Renormalization of the Stress Energy Tensor in a Spherically Symmetric Black Hole Space-Time with an Application to Lukewarm Black Holes

Details Hadamard Renormalization of the Stress Energy Tensor in a Spherically Symmetric Black Hole Space-Time with an Application to Lukewarm Black Holes Hadamard Renormalization of the Stress Energy Tensor in a Spherically Symmetric Black Hole Space-Time with an Application to Lukewarm Black Holes

2011-12-13

arxiv.org/abs/1112.3048v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

17 pages, 8 figures and 2 tables

Scientific paper

We consider a quantum field which is in a Hartle-Hawking state propagating in
a spherically symmetric black hole space-time. We calculate the components of
the stress tensor, renormalized using the Hadamard form of the Green's
function, in the exterior region of this space-time. We then specialize these
results to the case of the `lukewarm' Riessner-Nordstrom-de Sitter black hole.

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