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无截断薄膜模型与Dirac场的黑洞熵
  • 期刊名称:Acta Phys. Sin., (物理学报) (SCI Impact factor: 1.003)
  • 时间:0
  • 页码:060401-1-060401-7
  • 语言:中文
  • 分类:P145.8[天文地球—天体物理;天文地球—天文学] O316[理学—一般力学与力学基础;理学—力学]
  • 作者机构:[1]Department of Physics, Shaoxing University, Shaoxing 312000, China
  • 相关基金:Project supported by the National Natural Science Foundation of China (Grant No. 11045005) and the Natural Science Foundation of Zhejiang Province of China (Grant No. Y6090739).Acknowledgments The author would like to thank Dr. B. R. Majhi for useful suggestions and discussions.
  • 相关项目:黑洞量子隧穿辐射与信息疑难以及黑洞半经典量子化方案
作者: 杨学军|赵峥|
中文摘要:

By considering and using an adiabatic invariant for black holes, the area and entropy spectra of static spherically-symmetric black holes are investigated. Without using quasi-normal modes of black holes, equally-spaced area and entropy spectra are derived by only utilizing the adiabatic invariant. The spectra for non-charged and charged black holes are calculated, respectively. All these results are consistent with the original Bekenstein spectra.

英文摘要:

By considering and using an adiabatic invariant for black holes, the area and entropy spectra of static spherically- symmetric black holes are investigated. Without using quasi-normal modes of black holes, equally-spaced area and entropy spectra are derived by only utilizing the adiabatic invariant. The spectra for non-charged and charged black holes are calculated, respectively. All these results are consistent with the original Bekenstein spectra.

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