Absorption cross section of RN black hole
Abstract
Description
The behavior of a charged scalar field in the RN black hole space time is studied using WKB approximation. In the present work it is assumed that matter waves can get reflected from the event horizon. Using this effect, the Hawking temperature and the absorption cross section for RN black hole placed in a charged scalar field are calculated. The absorption cross section $σ_{abs}$ is found to be inversely proportional to square of the Hawking temperature of the black hole.
6 pages, 2 figures
6 pages, 2 figures