史瓦西黑洞残余的讨论

A Discussion on Schwarzschild Black Hole Remnant

本文运用负对数区域修正方法对史瓦西黑洞的Bekenstein-Hawking熵进行了分析,计算出了黑洞的逆温度和热容量,并且得到其临界质量。然后我们采用泰勒级数展开,讨论了史瓦西黑洞的隧穿概率,在对熵差进行计算的过程中,我们通过粒子的能量约束条件,解出了黑洞的最小临界质量。最后计算黑洞的隧穿概率,其结果分析得出黑洞残余与熵的修正有关,这将为黑洞残余的研究提供一种便捷的方法,并且可以避免黑洞的奇异性问题。

In this paper,the Bekenstein-Hawking entropy of Schwarzschild black hole is analyzed by using the negative logarithmic region correction method.The inverse temperature and thermal capacity of the black hole are calculated,and its critical mass is obtained.Then,Taylor series expansion is used to discuss the tunneling probability of Schwarzschild black hole.In the process of calculating the entropy difference,the minimum critical mass of the black hole is solved through the energy constraints of particles.Finally,the tunneling probability of the black hole is calculated,and the results show that the remnant of the black hole is related to the correction of the entropy.It will provide a convenient method for the research of the black hole,and avoid the singularity problem of the black hole.