Currents and radiation from the large D black hole membrane

被引:32
作者
Bhattacharyya, Sayantani [1 ]
Mandal, Anup Kumar [1 ]
Mandlik, Mangesh [2 ]
Mehta, Umang [3 ]
Minwalla, Shiraz [2 ]
Sharma, Utkarsh [4 ]
Thakur, Somyadip [2 ]
机构
[1] Indian Inst Technol, Dept Phys, Kanpur 208016, Uttar Pradesh, India
[2] Tata Inst Fundamental Res, Dept Theoret Phys, 1 Homi Bhabha Rd, Bombay 400005, Maharashtra, India
[3] Indian Inst Technol, Dept Phys, JVLR, Bombay 400076, Maharashtra, India
[4] Indian Inst Technol, Dept Elect Engn, JVLR, Bombay 400076, Maharashtra, India
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2017年 / 05期
关键词
Black Holes; Spacetime Singularities; FIELD-THEORIES;
D O I
10.1007/JHEP05(2017)098
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
It has recently been demonstrated that black hole dynamics in a large number of dimensions D reduces to the dynamics of a codimension one membrane propagating in flat space. In this paper we de fine a stress tensor and charge current on this membrane and explicitly determine these currents at low orders in the expansion in 1/D. We demonstrate that dynamical membrane equations of motion derived in earlier work are simply conservation equations for our stress tensor and charge current. Through the paper we focus on solutions of the membrane equations which vary on a time scale of order unity. Even though the charge current and stress tensor are not parametrically small in such solutions, we show that the radiation sourced by the corresponding membrane currents is generically of order 1/D-D D D. In this regime it follows that the 'near horizon' membrane degrees of freedom are decoupled from asymptotic flat space at every perturbative order in the 1/D expansion. We also define an entropy current on the membrane and use the Hawking area theorem to demonstrate that the divergence of the entropy current is point wise non negative. We view this result as a local form of the second law of thermodynamics for membrane motion.
引用
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页数:156
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