Schwarzschild-Tangherlini metric from scattering amplitudes in various dimensions

Stavros Mougiakakos, P. Vanhove
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引用次数: 27

Abstract

We derive the static Schwarzschild-Tangherlini metric by extracting the classical contributions from the multi-loop vertex functions of a graviton emitted from a massive scalar field. At each loop orders the classical contribution is proportional to a unique master integral given by the massless sunset integral. By computing the scattering amplitudes up to three-loop order in general dimension, we explicitly derive the expansion of the metric up to the fourth post-Minkowskian order $O(G_N^4)$ in four, five and six dimensions. There are ultraviolet divergences that are cancelled with the introduction of higher-derivative non-minimal couplings. The standard Schwarzschild-Tangherlini is recovered by absorbing their effects by an appropriate coordinate transformation induced from the de Donder gauge condition.
不同维度散射振幅的史瓦西-唐赫里尼度规
我们从一个大质量标量场发射的引力子的多环顶点函数中提取经典贡献,推导出静态史瓦西-坦赫里尼度规。在每个循环阶,经典贡献与由无质量日落积分给出的唯一主积分成正比。通过在一般维上计算三环阶的散射振幅,我们明确地推导出了在四维、五维和六维上至后闵可夫斯基阶O(G_N^4)$的度规展开式。由于引入了高导数非极小耦合,紫外线发散被抵消了。通过适当的由德东德规范条件引起的坐标变换,吸收它们的影响,恢复了标准的施瓦西-唐赫里尼。
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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