Interacting quantum fields in various charts of anti–de Sitter spacetime

E. Akhmedov, A. Artemev, I. Kochergin
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引用次数: 6

Abstract

The goal of the present note is to understand whether it is possible to define interacting quantum field theory in global anti de Sitter space-time with Lorentzian signature, in its covering space-time (whose time coordinate is not periodic) and in its Poincare patch. We show that in global anti de Sitter space-time there are certain problems to define quantum field theory properly. This is due to an additional UV singularity of the Feynman propagator which is sitting on the light-cone emanating from the antipodal point of the source. There is no such singularity in flat space-time. At the same time quantum field theory in Poincare region of the AdS space-time can be well defined and is related to the one in Euclidean AdS via the analytical continuation. In principle one can also define and analytically continue quantum field theory in the covering anti de Sitter space-time. However, to do that one has to use an unusual $i\epsilon$-prescription in the Feynman propagator, which cannot be used in loop calculations in non-stationary situations.
在各种反德西特时空图中相互作用的量子场
本笔记的目的是了解是否有可能在具有洛伦兹特征的全局反德西特时空中,在其覆盖时空(其时间坐标是非周期性的)中以及在其庞加莱补丁中定义相互作用量子场论。我们证明了在全局反德西特时空中量子场论的正确定义存在一些问题。这是由于费曼传播体的额外UV奇点,它位于从光源的对映点发出的光锥上。平坦时空中没有这样的奇点。同时,通过解析延拓,可以很好地定义ad时空庞加莱区域中的量子场论,并与欧几里得ad中的量子场论联系起来。原则上,我们也可以在覆盖的反德西特时空中定义和解析地延续量子场论。然而,要做到这一点,我们必须在费曼传播算子中使用一个不寻常的$i\ ε $-处方,它不能在非平稳情况下的循环计算中使用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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