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Entropy bound for the photon gas in noncommutative spacetime

机译:非交换时空中光子气体的熵约束

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摘要

Motivated by the doubly special relativity theories and noncommutative spacetime structures, thermodynamical properties of the photon gas in a phase space with compact spatial momentum space is studied. At the high temperature limit, the upper bounds for the internal energy and entropy are obtained which are determined by the size of the compact spatial momentum space. The maximum internal energy turns out to be of the order of the Planck energy and the entropy bound is then determined by the factor (V/l(pl)(3)) through the relevant identification of the size of the momentum space with Planck scale. The entropy bound is very similar to the case of Bekenstein-Hawking entropy of black holes and suggests that thermodynamics of black holes may be deduced from a saturated state in the framework of a full quantum gravitational statistical mechanics. (C) 2016 Elsevier B.V. All rights reserved.
机译:以双重相对论和非交换时空结构为动力,研究了光子气体在空间动量空间紧凑的相空间中的热力学性质。在高温极限下,获得内部能量和熵的上限,该上限由紧凑的空间动量空间的大小确定。最大内部能量证明是普朗克能量的量级,然后通过以普朗克尺度对动量空间的大小进行相关识别,由系数(V / l(pl)(3))确定熵界。熵界与黑洞的Bekenstein-Hawking熵的情况非常相似,并表明黑洞的热力学可能是在完全量子引力统计力学的框架内从饱和状态推导出来的。 (C)2016 Elsevier B.V.保留所有权利。

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