2015
DOI: 10.1103/physrevc.91.054907
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Relativistic quantum transport coefficients for second-order viscous hydrodynamics

Abstract: We express the transport coefficients appearing in the second-order evolution equations for bulk viscous pressure and shear stress tensor using Bose-Einstein, Boltzmann, and Fermi-Dirac statistics for the equilibrium distribution function and Grad's 14-moment approximation as well as the method of Chapman-Enskog expansion for the non-equilibrium part. Specializing to the case of transversally homogeneous and boost-invariant longitudinal expansion of the viscous medium, we compare the results obtained using the… Show more

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Cited by 63 publications
(72 citation statements)
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References 61 publications
(74 reference statements)
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“…This is different from the perturbative treatments of the weakly-coupled plasmas, which predict a quadratic scaling [49][50][51]. Surprisingly, our result seems to be in line with the results obtained in strongly-coupled theories using gauge theory/gravity duality [52][53][54].…”
Section: Bulk and Shear Viscosity And ζ/η Scalingsupporting
confidence: 68%
“…This is different from the perturbative treatments of the weakly-coupled plasmas, which predict a quadratic scaling [49][50][51]. Surprisingly, our result seems to be in line with the results obtained in strongly-coupled theories using gauge theory/gravity duality [52][53][54].…”
Section: Bulk and Shear Viscosity And ζ/η Scalingsupporting
confidence: 68%
“…For the sake of simplicity, we assume here the classical Boltzmann statistics. A generalisation of the present results to the case of the quantum Bose-Einstein and Fermi-Dirac statistics is straightforward [16,29]. The equilibrium distribution functions of the form (4) are used to define the RTA collision terms in (1) and (2).…”
Section: Kinetic Equationsmentioning
confidence: 99%
“…The calculation of such coefficients has attracted much attention lately (see [12] for a recent review), especially in conformal field theories [13][14][15] with different techniques [16,17] (see also ref. [18]). The coefficients that we have denoted by D α , D w , A and W are in the following relation with those known as ξ 3 , ξ 4 , λ 3 , λ 4 in literature:…”
Section: A Relation With Other Second-order Hydrodynamical Coefficiementioning
confidence: 99%