Vanishing Hawking Radiation from a Uniformly Accelerated Black Hole

Details Vanishing Hawking Radiation from a Uniformly Accelerated Black Hole Vanishing Hawking Radiation from a Uniformly Accelerated Black Hole

1995-03-26

arxiv.org/abs/gr-qc/9503047v2

Phys.Rev.Lett. 75 (1995) 382-385

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

LaTeX, 10pages, 2 figures (a typo in Eq.(3) corrected; minor revisions to accomodate the length limitation of the journal)

Scientific paper

10.1103/PhysRevLett.75.382

We consider quantum fields around uniformly accelerated black holes. At a particular value of the acceleration, the Bogolubov transformation which would be responsible for the late-time Hawking radiation, is found to be trivial. When this happens, Hawking's thermal radiation, Doppler-shifted or not, is absent to the asymptotic inertial observers despite the nonzero Hawking temperature, while the co-moving observers find the black hole radiance exactly balanced by the acceleration heat bath. After a brief comparison to the classical system of a uniformly accelerated charge, we close with two important comments. (Phys. Rev. Lett. 75 (1995) 382)

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