Hawking radiation in a fourdimensional pseudoRiemannian stationary spacetime
Abstract
We show that on the future horizon of a certain type of 4dimensional, stationary, pseudoRiemannian spacetime, Hawking radiation will generally be produced, with a temperature proportional to the surface gravity at the horizon. The Hawking radiations of the Schwarzschild, ReissnerNordstrom and KerrNewman blackholes 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.
 Publication:

Acta Astrophysica Sinica
 Pub Date:
 September 1983
 Bibcode:
 1983AcApS...3..146Z
 Keywords:

 Black Holes (Astronomy);
 KleinGordon Equation;
 Riemann Manifold;
 SpaceTime Functions;
 Thermal Radiation;
 Coordinate Transformations;
 Electromagnetic Fields;
 Extraterrestrial Radiation;
 Metric Space;
 Rotating Disks;
 Wave Equations;
 Astrophysics