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arXiv 1801.07489gr-qchep-th
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霍金辐射与Bloom-Gilman对偶性

Hawking radiation and the Bloom-Gilman duality

R. Casadio, A. Yu. Kamenshchik, O. V. Teryaev

摘要:

量子黑洞前体的衰变宽度,确定从极端的引力子传播,匹配的预期寿命给出的霍金衰变。通过这种方式,我们在微扰描述和本质上非微扰描述之间施加了一种对偶性,与强相互作用的Bloom-Gilman对偶性有一些相似之处。一般的关系,然后获得的宽度和质量的极的粒子种类的数量和重正化规模的重力。

英文摘要:

The decay widths of the quantum black hole precursors, determined from the poles of the resummed graviton propagator, are matched to the expected lifetime given by the Hawking decay. In this way, we impose a sort of duality between a perturbative description and an essentially non-perturbative description, bearing some similarity with the Bloom-Gilman duality for the strong interactions. General relations are then obtained for the widths and masses of the poles in terms of the number of particle species and the renormalisation scale of gravity.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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