2009
DOI: 10.1088/1126-6708/2009/12/066
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Stochastic string motion above and below the world sheet horizon

Abstract: Abstract:We study the stochastic motion of a relativistic trailing string in black hole AdS 5 . The classical string solution develops a world-sheet horizon and we determine the associated Hawking radiation spectrum. The emitted radiation causes fluctuations on the string both above and below the world-sheet horizon. In contrast to standard black hole physics, the fluctuations below the horizon are causally connected with the boundary of AdS. We derive a bulk stochastic equation of motion for the dual string a… Show more

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Cited by 26 publications
(31 citation statements)
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References 41 publications
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“…Such effective temperatures have been discussed previously (e.g., [30]) in the context of trailing strings [46,47], where a quark moving at equilibrium in a background plasma feels an effective temperature caused by a boost of the stress energy tensor in its frame. This leads to an effective temperature of the form…”
Section: Jhep06(2011)017mentioning
confidence: 78%
“…Such effective temperatures have been discussed previously (e.g., [30]) in the context of trailing strings [46,47], where a quark moving at equilibrium in a background plasma feels an effective temperature caused by a boost of the stress energy tensor in its frame. This leads to an effective temperature of the form…”
Section: Jhep06(2011)017mentioning
confidence: 78%
“…Later, the idea of this holographic duality has been extended to other systems such as strong coupling problems in condensed matter physics and the hydrodynamics of the quark-gluon plasma. Moreover, considerable efforts have been focused on using the holography idea to explore Brownian motion of a particle moving in a strongly coupled environment [31][32][33][34][35][36][37][38][40][41][42][43]. In addition, there have been extensive studies of above mentioned energy conditions with the holographic approach.…”
Section: Jhep09(2016)059mentioning
confidence: 99%
“…Then I(r) and K(r) in the metric perturbations are straightforwardly given by (2.34) with z = 1. Using the prescriptions (2.15) and (2.19), they leads to the boundary stress tensor to second order in gravitational wave perturbations, which is given by 36) where C can be determined by matching the black brane mass density to that of gravitational waves. As long as z = 2, the leading order results (2.35) in a large r expansion give nonvanishing stress tensor.…”
Section: Jhep09(2016)059mentioning
confidence: 99%
“…The authors of [60] focused on the case d = 4 and followed a different but equivalent route, employing the dual relation between the Kruskal extension of the Schwarzschild-AdS geometry and the CFT Schwinger-Keldysh formalism [61,62,7], together with the known connection between the latter and the generalized Langevin equation. These calculations were later generalized and elaborated on in [63,64,65,66].…”
Section: Late-time Energy Loss Brownian Motion and Limiting Velocitymentioning
confidence: 99%