The long string at the stretched horizon and the entropy of large non-extremal black holes

被引：17

作者：

Mertens, Thomas G. ^{[1
,2
]}

Verschelde, Henri ^{[2
]}

Zakharov, Valentin I. ^{[3
,4
,5
]}

机构：

[1] Princeton Univ, Joseph Henry Labs, Washington Rd, Princeton, NJ 08544 USA

[2] Univ Ghent, Dept Phys & Astron, Krijgslaan 281-S9, B-9000 Ghent, Belgium

[3] ITEP, B Cheremushkinskaya 25, Moscow 117218, Russia

[4] Moscow Inst Phys & Technol, Dolgoprudnyi 141700, Moscow Region, Russia

[5] Far Eastern Fed Univ, Sch Biomed, Sukhanova Str 8, Vladivostok 690950, Russia

来源：

JOURNAL OF HIGH ENERGY PHYSICS | 2016年 / 02期

关键词：

Black Holes in String Theory; Long strings; Tachyon Condensation; ORIGIN;

D O I：

10.1007/JHEP02(2016)041

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 discuss how long strings can arise at the stretched horizon and how they can account for the Bekenstein-Hawking entropy. We use the thermal scalar field theory to derive the asymptotic density of states and corresponding stress tensor of a microcanonical long string gas in Rindler space. We show that the equality of the Hagedorn and Hawking temperatures gives rise to the tree-level entropy of large black holes in accordance with the Bekenstein-Hawking-Wald formula.

引用

页码：1 / 18

页数：18

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