Some new properties of black holes in the quantum Oppenheimer-Snyder model
Shi-Hai DongCentro de Investigación en Computación, Instituto Politécnico Nacional, UPALM, CDMX 07700, MexicoFarokhnaz HosseinifarDepartment of Physics, Faculty of Science, University of Hradec Králové, Rokitanského 62, 500 03 Hradec Králové, CzechiaFilip StudničkaDepartment of Physics, Faculty of Science, University of Hradec Králové, Rokitanského 62, 500 03 Hradec Králové, CzechiaH. HassanabadiDepartment of Physics, Faculty of Science, University of Hradec Králové, Rokitanského 62, 500 03 Hradec Králové, Czechia
2024en
ABI
Аннотация
In response to the limitations of the classical Oppenheimer-Snyder model of black holes, we investigate the quantum framework proposed by Lewandowski et al. (2023) [29] . This quantum model incorporates corrections that allow for a detailed analysis of features such as black hole thermodynamics and Hawking radiation. In particular, we focus on the evaporation process and quasi-normal modes, utilizing the Rosen-Morse approximation method. Furthermore, we explore the topology of photon spheres and the thermodynamic topology of the black hole.
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