Abstract

We study parity-violating effects, particularly the generation of angular momentum density and its relation to the parity-odd and dissipationless transport coefficient Hall viscosity, in strongly-coupled quantum fluid systems in 2+1 dimensions using holographic method. We employ a class of 3+1-dimensional holographic models of Einstein-Maxwell system with gauge and gravitational Chern-Simons terms coupled to a dynamical scalar field. The scalar can condensate and break the parity spontaneously. We find that when the scalar condensates, a non-vanishing angular momentum density and an associated edge current are generated, and they receive contributions from both gauge and gravitational Chern-Simons terms. The angular momentum density does not satisfy a membrane paradigm form because the vector mode fluctuations from which it is calculated are effectively massive. On the other hand, the emergence of Hall viscosity is a consequence of the gravitational Chern-Simons term alone and it has membrane paradigm form. We present both general analytic results and numeric results which take back-reactions into account. The ratio between Hall viscosity and angular momentum density resulting from the gravitational Chern-Simons term has in general a deviation from the universal 1/2 value obtained from field theory and condensed matter physics.

Highlights

  • Vortex flow [18,19,20]

  • We study parity-violating effects, the generation of angular momentum density and its relation to the parity-odd and dissipationless transport coefficient Hall viscosity, in strongly-coupled quantum fluid systems in 2+1 dimensions using holographic method

  • We employ a class of 3+1-dimensional holographic models of EinsteinMaxwell system with gauge and gravitational Chern-Simons terms coupled to a dynamical scalar field

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Summary

Bulk and boundary actions

The bulk action of our holographic Chern-Simons model in 3+1 dimension is:. where Fμν = ∂μAν − ∂νAμ is the field strength of Maxwell field. The bulk action of our holographic Chern-Simons model in 3+1 dimension is:. The cosmological constant Λ = −3/L2 and L is the AdS radius. Though in the actual calculation we will try to keep V [θ] general and not to implement this form until we have to. Θ[θ] is a general functional of θ. We will try to keep its form general for as long as possible in our calculation. Where nμ is the outgoing unit normal 1-form of the boundary and γμν = gμν − nμnν is the induced metric on the boundary. There is a Chern-Simons boundary term, analog to Gibbons-Hawking term, added such that the Dirichlet boundary value problem is well posed:

Perturbative expansion of bulk action
Equations of motion and background
Formula for angular momentum density
Vector mode fluctuations and angular momentum density
Effective masses and membrane paradigm violation
Tensor mode fluctuations and Hall viscosity
Tensor mode EOMs and solutions
Numeric results of the axion condensate phase
Gravitational Chern-Simons model: the probe limit
Gravitational Chern-Simons model: including back-reactions
Gauge Chern-Simons model: angular momentum density
Conclusions and comments
Full Text
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