Thermodynamic Topology of Quantum RN Black Holes

Wen-Xiang Chen
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Abstract

This paper presents a comprehensive exploration of the thermodynamics of black holes, focusing on foundational concepts such as free energy, entropy, and topological numbers, alongside a detailed examination of quantum RN black holes. By extending the discussion to encompass the symmetry groups SO(2), SO(3)/SO(2), and SO(3) within the framework of (f(R)) gravity, the paper offers a nuanced understanding of black hole physics. Key insights include the pivotal role of free energy and entropy in understanding the thermodynamic properties of black holes, the significance of topological numbers in determining thermodynamic stability and phase transitions, and the implications of quantum mechanics and (f(R)) gravity on traditional thermodynamic concepts. This exploration not only enriches our theoretical knowledge of black holes but also sets the stage for future empirical investigations, marking a pivotal contribution to our ongoing quest to decipher the universe's mysteries.
量子 RN 黑洞的热力学拓扑学
本文对黑洞热力学进行了全面探讨,重点关注自由能、熵和拓扑数等基础概念,并对量子 RN 黑洞进行了详细研究。通过将讨论扩展到(f(R))引力框架内的对称组 SO(2)、SO(3)/SO(2) 和 SO(3),论文提供了对黑洞物理学的细致入微的理解。主要见解包括自由能和熵在理解黑洞热力学性质中的关键作用、拓扑数在决定热力学稳定性和相变中的意义,以及量子力学和(f(R))引力对传统热力学概念的影响。这些探索不仅丰富了我们对黑洞的理论知识,而且为未来的实证研究奠定了基础,为我们不断探索破解宇宙奥秘做出了重要贡献。
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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