The thermal scalar and random walks in curved spacetime

被引：0
|
作者：
Mertens, Thomas G. [1 ,2 ]
Verschelde, Henri [1 ]
Zakharov, Valentin I. [3 ,4 ,5 ]
机构：
[1] Univ Ghent, Dept Phys & Astron, Krijgslaan 281-S9, B-9000 Ghent, Belgium
[2] Princeton Univ, Joseph Henry Labs, Princeton, NJ 08544 USA
[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：
FORTSCHRITTE DER PHYSIK-PROGRESS OF PHYSICS | 2016年 / 64卷 / 4-5期
关键词：
String thermodynamics; Long strings; Black holes; BLACK-HOLES; STRINGS;
D O I：
10.1002/prop.201500056
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The curved space generalization of near-Hagedorn string thermodynamics is discussed in terms of the thermal scalar mode. This mode singly winds the compact time direction and represents the most dominating state near the Hagedorn temperature. We discuss the random walk picture in a curved background and its relation to the thermal scalar. Then we apply this formalism to the thermal gas near black hole horizons, where a long random walking string is found at string length from the black hole horizon, in agreement with Susskind's picture of the stretched membrane.
引用
收藏
页码：403 / 407
页数：5
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