Hessling's Quantum Equivalence Principle and the Temperature of an Extremal Reissner-Nordström Black Hole

Details Hessling's Quantum Equivalence Principle and the Temperature of an Extremal Reissner-Nordström Black Hole Hessling's Quantum Equivalence Principle and the Temperature of an Extremal Reissner-Nordström Black Hole

1995-10-10

arxiv.org/abs/gr-qc/9510016v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, standard LaTex, no figures

Scientific paper

The Hessling improvement of the Haag, Narnhofer and Stein principle is
analysed in the case of a massless scalar field propagating outside of an
extremal R-N black hole. It is found that this sort of ``Quantum (Einstein's)
Equivalence Principle'' selects only the R-N vacuum as a physically sensible
state, i.e., it selects the temperature $T=0$ only.

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