Fokker-Planck equation for black holes in thermal potential
نویسندگان
چکیده
We construct a kind of thermal potential and then put the black hole thermodynamic system in it. In this regard, some properties are related to geometric characteristics potential. Driven by intrinsic fluctuations, behavior is stochastic. With help solving Fokker-Planck equation analytically, we obtain discrete energy spectrum Schwarzschild Banados-Teitelboim-Zanelli (BTZ) holes For hole, proportional temperature ensemble, which an external parameter, ground state non-zero. BTZ only depends on AdS radius, parameter. Moreover, zero. This also reflects difference between three-dimensional gravity four-dimensional gravity.
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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.104.104022