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=1983acaps...3..146z&link_type=abstract

(Acta Astrophysica Sinica, vol. 3, no. 2, 1983, p. 146-158) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 7, Sept. 1

Astronomy and Astrophysics

Astronomy

12

Black Holes (Astronomy), Klein-Gordon Equation, Riemann Manifold, Space-Time Functions, Thermal Radiation, Coordinate Transformations, Electromagnetic Fields, Extraterrestrial Radiation, Metric Space, Rotating Disks, Wave Equations

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-Newman 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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