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中国物理学会期刊

量子史瓦茨黑洞和暗物质

CSTR: 32037.14.aps.55.4980

Quantum Schwarzschild black hole and dark matter

CSTR: 32037.14.aps.55.4980
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  • 引入Sommerfeld作用量量子化条件来处理Schwarzschild黑洞的量子化问题. 发现此类量子化黑洞存在一个质量为mG=123mp的基态,处于基态的量子Schwarzschild黑洞不再存在Hawking蒸发和任何其他辐射,可名之曰暗星. 它的存在不仅可以解决信息丢失的疑难,而且极可能是构成暗物质的主要候选者.

     

    If the situation of quantum gravity nowadays is nearly the same as that of quantum mechanics in its early time of Bohr and Sommerfeld, then a first-step study of the quantum gravity under Sommerfeld's quantum condition of action might be helpful. We present the spectra of quantum Schwarzschild black hole in non-relativistic quantum mechanics. It is found that the quantum of area is 8π3l2p, the quantum of entropy is 2π3kB, and the Hawking evaporation will cease when the black hole reaches the ground state m=123mp. A very natural conjecture is that the constituents of dark matter may come from the remnant (relics) of primordeal black hole with life time smaller than that of the universe.

     

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