Viscosity of holographic fluid in the presence of dark matter sector

Abstract

Based on the gauge/gravity correspondence, the hydrodynamic response coefficients, shear and Hall viscosities, have been studied. The holographic model of Einstein-Maxwell- AdS $(3+1)$-dimensional system additionally coupled with the another gauge field mimicking the {\it dark matter} sector, as well as, gravitational Chern-Simons term bounded with a dynamical scalar field, were taken into account. Condensation of the scalar field provides the parity violating term. Both shear and Hall viscosities have been calculated and their dependence on $\alpha$ - the coupling constant between matter and {\it dark matter} sectors has been studied. To the lowest order in the derivative expansion and perturbation in $\alpha$, the shear viscosity is not influenced by the {\it dark matter}, while the Hall component linearly depends on $\alpha$.

JHEP style, this version meets the published one, JHEP08 (2016) 124

References in corpus (26)

• Viscosity in Strongly Interacting Quantum Field Theories from Black Hole Physics
• Observation of an anomalous positron abundance in the cosmic radiation
• Nonlinear Fluid Dynamics from Gravity
• Viscosity Information from Relativistic Nuclear Collisions: How Perfect is the Fluid Observed at RHIC?
• Theory of the Nernst effect near quantum phase transitions in condensed matter, and in dyonic black holes
• Search for a dark photon in e+e- collisions at BABAR
• The non-gravitational interactions of dark matter in colliding galaxy clusters
• Viscosity Bound and Causality Violation
• Universal Quantum Viscosity in a Unitary Fermi Gas
• Search for ultralight scalar dark matter with atomic spectroscopy
• The behaviour of dark matter associated with 4 bright cluster galaxies in the 10kpc core of Abell 3827
• Worldline algorithms for Casimir configurations
• Viscous plasma evolution from gravity using AdS/CFT
• Resolving disagreement for eta/s in a CFT plasma at finite coupling
• Universal holographic hydrodynamics at finite coupling
• String Theory and Quantum Chromodynamics
• Detecting Dark Matter with Imploding Pulsars in the Galactic Center
• Viscosity bound violation in holographic solids and the viscoelastic response
• Dark Matter-induced Collapse of Neutron Stars: A Possible Link Between Fast Radio Bursts and the Missing Pulsar Problem
• Shear viscosity of boost invariant plasma at finite coupling
• A Strongly Coupled Anisotropic Fluid From Dilaton Driven Holography
• Particle dark matter searches outside the Local Group
• Shear viscosity of CFT plasma at finite coupling
• A particle dark matter footprint on the first generation of stars
• Hall Viscosity Revealed via Density Response
• Hall viscosity to entropy ratio in higher derivative theories

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