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Toward the New Gravitational Noncommutative Mechanics and Statistical Mechanics of Quantum Black Holes

机译:走向新引力非交换力学与统计学   量子黑洞力学

摘要

This is a short account of our work on the statistical mechanics of `cold'quantum black holes in the constituent model of a black hole$^{3,4,6}$. Aquantum Schwarzschild black hole consists of gravitational atoms of Planckianmass scale$^{3,4,6}$. The gapless collective excitations of a bound state of Ngravitational atoms dominate the thermodynamics of a cold quantum black hole.It turns out that it is only in the limit of large $N$, with the observablemean values of the gravitational mass-energy kept fixed, that we recover theBekenstein thermodynamics$^1$ of spin-zero black holes. This is also the limitof the Boltzmann statistics.
机译:这是我们对黑洞$ ^ {3,4,6} $的构成模型中“冷”量子黑洞的统计力学所做的工作的简短说明。 Aquantum Schwarzschild黑洞由Planckianmass尺度$ ^ {3,4,6} $的引力原子组成。引力原子的束缚态的无隙集体激发支配着冷量子黑洞的热力学,事实证明它仅在$ N $的极限内,引力质量能的可观测平均值保持固定,我们恢复了自旋零黑洞的贝肯斯坦热力学$ ^ 1 $。这也是玻耳兹曼统计的极限。

著录项

  • 作者

    Mazur, P. O.;

  • 作者单位
  • 年度 1998
  • 总页数
  • 原文格式 PDF
  • 正文语种 {"code":"en","name":"English","id":9}
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