Hawking radiation and the Bloom-Gilman duality

被引:1
作者
Casadio, R. [1 ,2 ]
Kamenshchik, Alexander Yu [1 ,2 ,3 ]
Teryaev, Oleg, V [4 ,5 ,6 ]
机构
[1] Dipartimento Fis & Astron, Via Irnerio 46, I-40126 Bologna, Italy
[2] INFN, Via Irnerio 46, I-40126 Bologna, Italy
[3] Russian Acad Sci, LD Landau Inst Theoret Phys, Kosygin Str 2, Moscow 119334, Russia
[4] Joint Inst Nucl Res, Dubna 141980, Russia
[5] Dubna Int Univ, Dubna 141980, Russia
[6] Lomonosov Moscow State Univ, Leninskie Gory 1, Moscow 119991, Russia
关键词
black holes; duality; graviton propagator; SCALE; QCD;
D O I
10.1088/1361-6382/aacc55
中图分类号
P1 [天文学];
学科分类号
0704 ;
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 kind 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. A lower bound on the lifetime of the quantum black holes is also obtained.
引用
收藏
页数:8
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