黑洞的修正热力学在 (f) 重力与电动场和宇宙常数的重力
Mou Xu1, Yuying Zhang1, Liu Yang1
1Department of Physics, Liaoning Normal University, Dalian 116029, China.
Entropy (Basel, Switzerland)
|October 25, 2024
概括
这项研究探讨了f (R) 重力模型中的修正黑洞热力学. 热波动显著影响小黑洞的和自由能量,确保局部稳定性和霍金-佩奇相位过渡.
科学领域:
- 引力物理 引力物理
- 黑洞热力学 黑洞热力学
- 修改引力理论 修改引力理论
背景情况:
- 黑洞热力学和纠正在引力物理学中至关重要.
- f) 重力理论为广义相对论提供了替代模型.
研究的目的:
- 在f(R) =R+αR2和f(R) =R+2γR+8Λ模型中研究黑洞的热力学和校正.
- 分析热波动对黑洞和热力学量的影响.
主要方法:
- 在f ((R)) 理论下研究了球形对称的黑洞,并使用了电动场和宇宙常数.
- 考虑在平衡状态周围的热波动.
- 利用特定热量推导出纠正的热力学量,并分析黑洞的稳定性.
主要成果:
- 纠正的对于负宇宙常数 (反de Sitter-RN时空) 有意义.
- 热波动显著影响小黑洞的.
- 对于小黑洞来说,对赫尔姆霍尔茨和吉布斯自由能量的修正是值得注意的.
- 黑洞热力学表现出局部稳定性,并经历霍金-佩奇相位过渡.
结论:
- 具有热波动的重力模型提供了稳定的黑洞解决方案.
- 该研究限制了爱因斯坦-希尔伯特半径的非负黑洞体积.
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