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Some new properties of black holes in the quantum Oppenheimer-Snyder model
Physics Letters B ( IF 4.3 ) Pub Date : 2024-12-10 , DOI: 10.1016/j.physletb.2024.139182
Shi-Hai Dong, Farokhnaz Hosseinifar, Filip Studnička, Hassan Hassanabadi

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.

中文翻译:


量子 Oppenheimer-Snyder 模型中黑洞的一些新性质



为了应对经典的 Oppenheimer-Snyder 黑洞模型的局限性,我们研究了 Lewandowski 等人(2023 年)提出的量子框架 [29]。该量子模型包含校正,允许对黑洞热力学和霍金辐射等特征进行详细分析。特别是,我们利用 Rosen-Morse 近似方法关注蒸发过程和准正态模式。此外,我们探索了光子球的拓扑结构和黑洞的热力学拓扑。
更新日期:2024-12-10
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