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arXiv hep-th/0209067hep-th
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全息重整化讲义

Lecture Notes on Holographic Renormalization

Kostas Skenderis

摘要:

我们回顾了全息重整化的形式。我们首先讨论渐近反德西特时空的数学结果。然后,我们概述了全息重整化的一般方法。这个方法是通过一个简单的例子来说明的:反德西特时空上的大质量标量场。讨论内容包括在壳重正化作用量、全息沃德恒等式、反常和RG方程的推导,以及重正化一点、二点和四点函数的计算。然后,我们讨论了全息RG流的方法的应用。我们还表明,渐近AdS时空的近边界分析的结果可以解析地继续适用于渐近de Sitter时空。特别是,它表明,布朗约克应力能量张量的德西特时空是相等的,直到一个维度相关的符号,布朗约克应力能量张量的相关AdS时空。

英文摘要:

We review the formalism of holographic renormalization. We start by discussing mathematical results on asymptotically anti-de Sitter spacetimes. We then outline the general method of holographic renormalization. The method is illustrated by working all details in a simple example: a massive scalar field on anti-de Sitter spacetime. The discussion includes the derivation of the on-shell renormalized action, of holographic Ward identities, anomalies and RG equations, and the computation of renormalized one-, two- and four-point functions. We then discuss the application of the method to holographic RG flows. We also show that the results of the near-boundary analysis of asymptotically AdS spacetimes can be analytically continued to apply to asymptotically de Sitter spacetimes. In particular, it is shown that the Brown-York stress energy tensor of de Sitter spacetime is equal, up to a dimension dependent sign, to the Brown-York stress energy tensor of an associated AdS spacetime.

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