2014
DOI: 10.1103/physrevd.89.064036
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Holographic parity-violating charged fluid dual to Chern-Simons modified gravity

Abstract: We discuss the (2 þ 1)-dimensional parity-violating charged fluid on a finite cutoff surface Σ c , dual to the nondynamical and dynamical Chern-Simons (CS) modified gravities. Using the nonrelativistic longwavelength expansion method, the field equations are solved up to Oðϵ 2 Þ in the nondynamical model. It is shown that there exists nonvortical dual fluid with shear viscosity η and Hall viscosity η A on the cutoff surface Σ c . The ratio of shear viscosity over entropy density η=s of the fluid takes the univ… Show more

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Cited by 9 publications
(14 citation statements)
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“…This relation has been well established in the context of quantum Hall effects using other methods [29,30,47,49], but not confirmed from the Chern-Simons effective theory as far as we know, including in holography [139][140][141][142][143][144][145][146][147]. 4 We distinguish two types of angular momentum densities from the Chern-Simons effective theory and show that how the above relation arises (Section 5).…”
Section: Outline and Notationsmentioning
confidence: 86%
“…This relation has been well established in the context of quantum Hall effects using other methods [29,30,47,49], but not confirmed from the Chern-Simons effective theory as far as we know, including in holography [139][140][141][142][143][144][145][146][147]. 4 We distinguish two types of angular momentum densities from the Chern-Simons effective theory and show that how the above relation arises (Section 5).…”
Section: Outline and Notationsmentioning
confidence: 86%
“…19 Hall viscosity has been studied extensively in the context of Holography, e.g. see [58][59][60][61][62][63][64]69] where C mn is the Cotton-York tensor (4.15). Therefore, following [66], the Θ-term contribution to the energy-momentum tensor of the dual field theory is given by 20…”
Section: Energy-momentum Tensormentioning
confidence: 99%
“…where T (GB) ab is the one given in (6). Notice that P (α) ab in (35) has become the hypersurface function of extrinsic curvature K ab , but it is not true for δP (H) ab in (36). For example, we can see from [60] that the term…”
Section: Petrov Type I Condition On the Hypersurface σ Cmentioning
confidence: 99%
“…whereK ab is the contribution from vacuum Einstein gravity, and δK (α) ab includes the terms from the Gauss-Bonnet term at first order in small α expansion. Then from (35)…”
Section: Petrov Type I Condition On the Hypersurface σ Cmentioning
confidence: 99%
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