论文标题

量子黑洞是什么样的?

What does a quantum black hole look like?

论文作者

Aoki, Sinya, Onogi, Tetsuya, Yokoyama, Shuichi

论文摘要

我们通过流动方程式迈出了对黑洞的全息描述的第一步。我们考虑了有限温度下多个标量场的自由理论,并研究了通过标量场的自由流量定义的全息几何学。我们发现全息照相指标具有以下特性:i)它是一个渐近抗DE保姆(ADS)黑色brane公制,具有一些未知物质的贡献。 ii)它没有坐标的奇异性和温和的曲率奇异性。 iii)其时间成分在某个ADS径向切片上成倍衰减。我们发现,此物质在整个空间中扩散,我们推测这是由于无限许多无质量高的自旋场的热激发所致。我们猜想上面的三个是流动方程方法实现的黑洞全息的通用特征。

We take a first step towards a holographic description of a black hole by means of a flow equation. We consider a free theory of multiple scalar fields at finite temperature and study its holographic geometry defined through a free flow of the scalar fields. We find that the holographic metric has the following properties: i) It is an asymptotic Anti-de Sitter (AdS) black brane metric with some unknown matter contribution. ii) It has no coordinate singularity and milder curvature singularity. iii) Its time component decays exponentially at a certain AdS radial slice. We find that the matter spreads all over the space, which we speculate to be due to thermal excitation of infinitely many massless higher spin fields. We conjecture that the above three are generic features of a black hole holographically realized by the flow equation method.

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