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Uncertainty relation and black-hole entropy of NUT-Kerr-Newman space-time

机译:NUT-Kerr-Newman时空的不确定性关系和黑洞熵

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摘要

In this paper, by using the quantum-statistical method and the new equation of state density motivated by the generalized uncertainty relation in the quantum gravity, we directly obtain the partition function of the Bose field and the Fermi field on the background of the axisymmetrical NUT-Kerr-Newman black hole. Then we calculate the entropy of the Bose field and the Fermi field of the black hole near the horizon. And it is obtained that the entropy of the black hole is proportional to the area of the horizon. The inherent contact between the entropy of the black hole and the area of the horizon is opened out. It is shown the entropy of the black hole is the entropy of the quantum state on the surface of the horizon. The entropy is a quantum effect. The fact that the state density diverges near the horizon is removed by introducing the generalized uncertainty relation showing that the brick-wall method is related to quantization of the quantum field.
机译:本文采用量子统计方法和量子引力中广义不确定性关系所激发的新的状态密度方程,直接得到轴对称NUT背景下Bose场和Fermi场的分配函数。 -Kerr-Newman黑洞。然后,我们计算了地平线附近黑洞的Bose场和Fermi场的熵。并且获得黑洞的熵与地平线的面积成比例。揭示了黑洞的熵与地平线区域之间的内在联系。可以看出黑洞的熵是地平线表面上量子态的熵。熵是量子效应。通过引入广义不确定性关系消除了状态密度在地平线附近发散的事实,该关系表明砖墙方法与量子场的量化有关。

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