爱因斯坦-非线性麦克斯韦-汤川黑洞中的热量子涨落
Thermal Quantum Fluctuations in Einstein-Nonlinear Maxwell-Yukawa Black Hole
浏览论文内容
中文总结 AI 辅助
本研究针对汤川屏蔽电磁势产生的爱因斯坦-非线性麦克斯韦-汤川黑洞，通过两种熵修正项分析不同视界尺度下的热涨落效应，探究其热力学行为与稳定性。
中文摘要 AI 辅助
本研究探究由汤川屏蔽电磁势产生的爱因斯坦-非线性电动力学黑洞，并通过计算基本热力学势与变量考察其热性质。针对贝肯斯坦-霍金熵添加的两种不同修正项，分析热涨落对所计算标准热力学量的影响：其一，采用代表恒定背景下量子场修正的对数修正项，研究事件视界相对较大时黑洞的热力学行为；其二，采用反映非微扰量子效应的指数修正项，分析事件视界较小时出现的热涨落。最后，对所有所得情形的热力学函数进行图形化考察，并详细讨论黑洞的稳定性性质。
英文摘要
This study investigates an Einstein-nonlinear electrodynamic black hole generated by a Yukawa-screened electromagnetic potential and examines its thermal properties through the calculation of the fundamental thermodynamic potentials and variables. The effect of thermal fluctuations on the calculated standard thermodynamic quantities is analyzed through two different correction terms added to the Bekenstein-Hawking entropy. In this work, the thermodynamic behavior in cases where the black hole has a relatively large event horizon is investigated using a logarithmic correction term representing corrections arising from quantum fields in constant backgrounds. In addition, thermal fluctuations occurring in cases where the event horizon is small are analyzed through an exponential correction term added to the entropy, reflecting non-perturbative quantum effects. Finally, the thermodynamic functions for all obtained cases are examined graphically, and the stability properties of the black hole are discussed in detail.
发表机构
- Eastern Mediterranean University（东地中海大学）
机构由 AI 辅助整理，请以论文原文为准。
