Proper time to the black hole singularity from thermal one-point functions

被引：49

作者：

Grinberg, Matan ^{[1
,2
]}

Maldacena, Juan ^{[3
]}

机构：

[1] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA

[2] Univ Cambridge, Dept Appl Math & Theoret Phys, Cambridge, England

[3] Inst Adv Study, Olden Lane, Princeton, NJ 08540 USA

来源：

JOURNAL OF HIGH ENERGY PHYSICS | 2021年 / 2021卷 / 03期

关键词：

AdS-CFT Correspondence; Spacetime Singularities; Black Holes in String Theory; Conformal Field Theory;

D O I：

10.1007/JHEP03(2021)131

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

We argue that the proper time from the event horizon to the black hole singularity can be extracted from the thermal expectation values of certain operators outside the horizon. This works for fields which couple to higher-curvature terms, so that they can decay into two gravitons. To extract this proper time, it is necessary to vary the mass of the field.

引用

页数：31

共 34 条

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JOURNAL OF HIGH ENERGY PHYSICS, 2015, (08):
[32] Scrambling time from local perturbations of the eternal BTZ black hole
Pawel Caputa
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[33] Black hole excited states from broken translations in Euclidean time
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JOURNAL OF HIGH ENERGY PHYSICS, 2024, 2024 (01)
[34] One-point functions in β-deformed N=4\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathcal{N}=4 $$\end{document} SYM with defect
Erik Widén
Journal of High Energy Physics, 2018 (11)

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