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Entropy and area in loop quantum gravity

机译:环量子引力的熵和面积

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Black hole thermodynamics suggests that the maximum entropy that can be contained in a region of space is proportional to the area enclosing it rather than its volume. We argue that this follows naturally from loop quantum gravity and a result of Kolmogorov and Bardzin' on the the realizability of networks in three dimensions. This represents an alternative to other approaches in which some sort of correlation between field configurations helps limit the degrees of freedom within a region. It also provides an approach to thinking about black hole entropy in terms of states inside rather than on its surface. Intuitively, a spin network complicated enough to imbue a region with volume only lets that volume grow as quickly as the area bounding it.
机译:黑洞热力学表明,一个空间区域中可以包含的最大熵与包围它的面积成正比,而不是与其体积成正比。我们认为,这自然是由于环量子引力以及Kolmogorov和Bardzin在三个维度上实现网络的结果所致。这代表了其他方法的替代方法,在这些方法中,场配置之间的某种相关性有助于限制区域内的自由度。它还提供了一种根据内部而不是表面状态来考虑黑洞熵的方法。直观地讲,自旋网络足够复杂,无法向具有体积的区域注入能量,这只能使该体积的增长速度与其包围区域的速度一样快。

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