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arXiv 1409.4498hep-thgr-qc
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关于模糊球面积谱、黑洞光度和时空量子性质的注记

A note on the fuzzy sphere area spectrum, black hole luminosity, and the quantum nature of spacetime

Victor Santos, C. A. S. Silva, C. A. S. Almeida

摘要:

通过对模糊球的热核迹进行渐近展开,得到了对模糊球面积经典表达式的非对易修正。作为一个重要的结果,黑洞的光度一定会出现某些量子引力偏差。我们计算这些偏差的静态,球对称,黑洞的视界模型的模糊球。所获得的结果可以通过大型强子对撞机(LHC)中形成的黑洞的辐射来验证。

英文摘要:

Non-commutative corrections to the classical expression for the fuzzy sphere area are found out through the asymptotic expansion for its heat kernel trace. As an important consequence, some quantum gravity deviations in the luminosity of black holes must appear. We calculate these deviations for a static, spherically symmetric, black-hole with a horizon modeled by a fuzzy sphere. The results obtained could be verified through the radiation of black holes formed in the Large Hadron Collider (LHC).

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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