Quantum Thermal Effect of Nonstatic Charged Black Hole

Authors: Lichun Z.; Yueqin W.; Ren Z.

Source: International Journal of Theoretical Physics, Volume 38, Number 2, 1 February 1999 , pp. 665-673(9)

Publisher: Springer

Abstract:

The difficulty of calculating energy-momentum tensors is avoided by finding directly the solution of Klein–Gordon and Dirac equations near the horizon. Both the location of the event horizon and the Hawking radiation temperature of a nonstatic charged black hole are shown. The results indicate that the Hawking radiation temperature can be regarded as a compensating effect under the timescale transformation.

Language: English

Document Type: Regular paper

Publication date: 1999-02-01

• In this: publication
• By this: publisher
• In this Subject: Physics (General)
• By this author: Lichun Z. ;  Yueqin W. ;  Ren Z.

Website © Publishing Technology. Article copyright remains with the publisher, society or author(s) as specified within the article.

• Terms and conditions
• Privacy policy
• Information for advertisers