Compactified AdS black holes, Chamblin-Reall background, and their dual non-conformal relativistic fluids
Chao Wu, Yanqi Wang

TL;DR
This paper derives all second-order transport coefficients for relativistic fluids dual to compactified AdS black holes, demonstrating their Chamblin-Reall background origin, generalizing previous results across dimensions, and analyzing the Kanitscheider-Skenderis proposal.
Contribution
It provides a comprehensive derivation of second-order transport coefficients for fluids dual to compactified AdS black holes and establishes their Chamblin-Reall background connection across dimensions.
Findings
All analytical second-order transport coefficients originate from Chamblin-Reall backgrounds.
Generalization of second-order transport coefficients to arbitrary dimensions.
Validation and physical interpretation of the Kanitscheider-Skenderis proposal.
Abstract
The Chamblin-Reall background is a static solution of Einstein gravity coupled with a background scalar field and a dynamical domain wall, with the potential of the scalar field being of Liouville type. It can be got by dimensionally reducing a higher dimensional background with a constant potential. Compactified AdS black holes are black hole backgrounds constructed by wrapping one or more spatial directions of a higher dimensional AdS black hole on a torus and then integrating them out. The compactified AdS black hole background is asymptotically flat, non-conformal, and of Chamblin-Reall type. In this work, we derive all the 7 dynamical second-order transport coefficients for the relativistic fluids dual to compactified AdS black holes of various dimensions via fluid/gravity correspondence. Through this work, we achieve three main goals: (1) We prove that all the gravitational…
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