计算正态黑洞准正态模式和拓扑电荷的新方法

arXiv - PHYS - General Relativity and Quantum Cosmology Pub Date : 2024-08-08 DOI:arxiv-2408.04704

MY Zhang, F Hosseinifar, H Chen, T Sathiyaraj, H Hassanabadi

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引用次数: 0

摘要

本研究探讨了一个特殊规则黑洞的特性。该分析研究了霍金温度、残余半径和质量，以及参数$\xi$对熵、热容量和自由能等热力学量的影响。此外，还探讨了黑洞的发射率、蒸发过程、通过计算罗森-莫尔斯势的准正态模以及拓扑行为。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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A New Approach for Calculation of Quasi-Normal Modes and Topological Charges of Regular Black Holes

This study examines the properties of a special regular black hole. This analysis investigates the Hawking temperature, remnant radius and mass, as well as the effect of parameter $\xi$ on thermodynamic quantities like entropy, heat capacity, and free energy. The emission rate, evaporation process, quasi-normal modes by calculating Rosen-Morse potential, and topological behavior of the black hole are also explored.

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arXiv - PHYS - General Relativity and Quantum Cosmology

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