Hawking radiation in a four-dimensional pseudo-riemannian stationary spacetime

Details Hawking radiation in a four-dimensional pseudo-riemannian stationary spacetime Hawking radiation in a four-dimensional pseudo-riemannian stationary spacetime

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983cha%26a...7..201z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 7, Issue 3, p. 201-210.

Astronomy and Astrophysics

Astrophysics

10

Scientific paper

We show that on the future horizon of a certain type of 4-dimensional, stationary, pseudo-Riemannian spacetime, Hawking radiation will generally be produced, with a temperature proportional to the surface gravity at the horizon. The Hawking radiations of the Schwarzschild, Reissner-Nordstrom and Kerr-Mewman black-holes and the de Sitter universe appear as particular instances of our proof. Unlike a uniformly accelerated detector, a uniformly rotating detector cannot detect Rindler radiation

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