Hawking effect of the Dirac particle in spherically symmetric nonstatic charged space time. (Chinese. English summary) Zbl 0952.83026
Summary: The difficulty of calculating energy-momentum tensors is avoided by finding directly the solution of Dirac equations near the horizon. Both the location of the event horizon and Hawking radiation temperature of a nonstatic charged spherically symmetric black hole are shown. The results indicate that the Hawking radiation temperature can be regarded as a compensating effect under the time scale transformation.
MSC:
| 83C57 | Black holes |
| 80A10 | Classical and relativistic thermodynamics |
| 83C60 | Spinor and twistor methods in general relativity and gravitational theory; Newman-Penrose formalism |
| 83C50 | Electromagnetic fields in general relativity and gravitational theory |
