全文下载：2012030328
郭广海
( 青岛科技大学 数理学院，山东 青岛266061)
摘要: 分别采用Maggiore和Kunstatter的方法，利用极端RN黑洞的似正规模计算了此黑洞的贝肯斯坦-霍金熵量子谱。结果表明，极端RN黑洞的熵量子谱是等间距的，而且所得的结论与贝肯斯坦的结果一致，但不同于Setare从Hod猜想所得的结果。
关键词: 贝肯斯坦-霍金熵；似正规模；极端RN黑洞
中图分类号: O 412.3文献标志码： A
Quantum Spectrum of Bekenstein-Hawking Entropy of the Extreme RN Black Hole
GUO Guang-hai
（College of Mathematics and Physics，Qingdao University of Science and Technology，Qingdao 266061, China）
Abstract: The quantum spectrum of Bekenstein-Hawking entropy of the extreme RN black hole is calculated with Maggiore’s and Kunstatter’s methods respectively, where the quasinormal modes of the black hole are employed. It is found that the quantum spectrum of the entropy is equidistant, and the results are consistent with Bekenstrin's but different from the results of Setare from Hod’s conjecture.
Key words: Bekenstein-Hawking entropy; quasinormal modes; RN extreme black hole
收稿日期:2011-12-29
作者简介: 郭广海(1976—)，男，副教授.
