Quasinormal modes and microscopic structure of the Schwarzschild black hole
نویسندگان
چکیده
Maggiore observed that, in the high-damping regime, quasi-normal modes spectrum for Schwarzschild black hole resembles that of a quantum harmonic oscillator. Motivated by this observation, we describe as statistical ensemble N oscillators. By working canonical ensemble, show large-mass limit, leading contribution to Gibbs entropy is Bekenstein-Hawking term, while subleading one logarithmic correction, agreement with several results literature. We also find number oscillators scales holographically area event horizon.
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ژورنال
عنوان ژورنال: Physical review
سال: 2021
ISSN: ['0556-2813', '1538-4497', '1089-490X']
DOI: https://doi.org/10.1103/physrevd.104.l121502