基于绝热不变性的黑洞谱学
Black hole spectroscopy via adiabatic invariance
摘要：
近年来，为了导出几个黑洞的量子化熵谱及其最小变化，人们不得不将准正规频率与黑洞的关系和黑洞的绝热不变性结合起来。本文利用黑洞视界面积是绝热不变量的命题，导出了量子等于Bekenstein给出的黑洞的等间距熵谱。有趣的是，在我们的方法中不需要准正态模式的概念。
英文摘要：
During the last years, one had to combine the proposal about how quasinormal frequencies are related with black holes and the proposal about the adiabatic invariance of black holes in order to derive the quantized entropy spectrum and its minimum change for several black holes. In this letter we exclusively utilize the statement that the black hole horizon area is an adiabatic invariant and derive an equally spaced entropy spectrum of a black hole with its quantum to be equal to the one given by Bekenstein. Interestingly, in our approach no concept of quasi-normal mode is needed.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
