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中国物理学会期刊

Schwarzschild-de-Sitter黑洞宇宙视界量子态的熵

CSTR: 32037.14.aps.53.3270

The quantum state entropy of Schwarzchild-de Sitter black hole cosmos horizon

CSTR: 32037.14.aps.53.3270
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  • 采用由广义不确定关系得到的新的态密度方程,研究了Schwarzchild-de-Sitter时空背景下黑洞宇宙视界的熵.利用新的态密度方程,克服了用brickwall模型方法计算黑洞熵,在消除紫外发散需取截断的不完善之处,以此揭示了黑洞熵与其视界面积成正比这一内在联系,进一步表明黑洞熵是视界面处量子态的熵.

     

    Using the new equation for density of states due to the generalized uncertainty relation, the entropy of Schwarzchildde Sitter spacetime is discussed. By use of the new equation for density of states, it overcomes the shortcoming that on eliminating divergence the calculation of black hole entropy with brickwall pattern needs a cut off. Thus, it gets the result of the direct proportion betwee n black hole entropy and its horizon area, brings to light the relationship between Schwarzchildde Sitter and its cosmos event horizon and makes clear that the black hole entropy is the entropy of quantum state near the event horizon.

     

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