Fluctuation and dissipation in de Sitter space

被引:27
作者
Fischler, Willy [1 ,2 ]
Nguyen, Phuc H. [2 ,3 ]
Pedraza, Juan F. [1 ,2 ]
Tangarife, Walter [1 ,2 ]
机构
[1] Univ Texas Austin, Dept Phys, Theory Grp, Austin, TX 78712 USA
[2] Univ Texas Austin, Texas Cosmol Ctr, Austin, TX 78712 USA
[3] Univ Texas Austin, Dept Phys, Ctr Relat, Austin, TX 78712 USA
基金
美国国家科学基金会;
关键词
AdS-CFT Correspondence; Long strings; Stochastic Processes; Quantum Dissipative Systems; HOLOGRAPHIC BROWNIAN-MOTION; N GAUGE-THEORY; HEAVY QUARKS; WILSON LOOPS; BLACK-HOLE; DIFFUSION; RENORMALIZATION; PHYSICS; LIMIT; MODEL;
D O I
10.1007/JHEP08(2014)028
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
In this paper we study some thermal properties of quantum field theories in de Sitter space by means of holographic techniques. We focus on the static patch of de Sitter and assume that the quantum fields are in the standard Bunch-Davies vacuum. More specifically, we follow the stochastic motion of a massive charged particle due to its interaction with Hawking radiation. The process is described in terms of the theory of Brownian motion in inhomogeneous media and its associated Langevin dynamics. At late times, we find that the particle undergoes a regime of slow diffusion and never reaches the horizon, in stark contrast to the usual random walk behavior at finite temperature. Nevertheless, the fluctuation-dissipation theorem is found to hold at all times.
引用
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页数:42
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