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arXiv 0803.4087hep-thgr-qcquant-ph
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场论中的重整化热熵

Renormalized Thermal Entropy in Field Theory

Sergio Cacciatori, Fabio Costa, Federico Piazza

摘要:

量子场论中的标准熵计算,当应用到一个子系统的确定体积,表现出面积依赖的紫外发散,使热力学解释麻烦。本文定义了一个与Newton-Wigner位置算符有关的重整化熵。因此,每当我们在空间区域上追踪时,我们追踪的自由度是根据牛顿-维格纳局部化而不是通常意义上的局部化的。我们考虑一个自由的标量场在d+1时空维度准备在热态,我们表明,我们的熵是免费的发散,并有一个完美的声音热力学行为。在高温/大体积极限下,我们的结果与标准QFT计算一致,只要从后者中减去发散贡献。在低温/小体积的极限下,熵趋于零,但对温度的依赖性不同。

英文摘要:

Standard entropy calculations in quantum field theory, when applied to a subsystem of definite volume, exhibit area-dependent UV divergences that make a thermodynamic interpretation troublesome. In this paper we define a renormalized entropy which is related with the Newton-Wigner position operator. Accordingly, whenever we trace over a region of space, we trace away degrees of freedom that are localized according to Newton-Wigner localization but not in the usual sense. We consider a free scalar field in d+1 spacetime dimensions prepared in a thermal state and we show that our entropy is free of divergences and has a perfectly sound thermodynamic behavior. In the high temperature/big volume limit our results agree with the standard QFT calculations once the divergent contributions are subtracted from the latter. In the limit of low temperature/small volume the entropy goes to zero but with a different dependence on the temperature.

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