Dissipative superfluid dynamics from gravity

TL;DR

This paper constructs a gravitational dual to dissipative superfluid dynamics by perturbing charged black branes in AdS space, deriving explicit first-order dissipative corrections, and extending existing fluid dynamic frameworks.

Contribution

It generalizes Herzog's infinite charge analysis by perturbing away from infinite charge, creating a detailed gravitational model of dissipative superfluid dynamics with 14 parameters.

Findings

Derived explicit metric, gauge, and scalar fields for superfluid flows.

Computed all dissipative constants for gravitational superfluids.

Extended the superfluid equations beyond Clark-Putterman's 13-parameter framework.

Abstract

Charged asymptotically AdS black branes in five dimensions are sometimes unstable to the condensation of charged scalar fields. For fields of infinite charge and squared mass -4 Herzog was able to analytically determine the phase transition temperature and compute the endpoint of this instability in the neighborhood of the phase transition. We generalize Herzog's construction by perturbing away from infinite charge in an expansion in inverse charge and use the solutions so obtained as input for the fluid gravity map. Our tube wise construction of patched up locally hairy black brane solutions yields a one to one map from the space of solutions of superfluid dynamics to the long wavelength solutions of the Einstein Maxwell system. We obtain explicit expressions for the metric, gauge field and scalar field dual to an arbitrary superfluid flow at first order in the derivative expansion. Our construction allows us to read off the the leading dissipative corrections to the perfect superfluid stress tensor, current and Josephson equations. A general framework for dissipative superfluid dynamics was worked out by Landau and Lifshitz for zero superfluid velocity and generalized to nonzero fluid velocity by Clark and Putterman. Our gravitational results do not fit into the 13 parameter Clark-Putterman framework. Purely within fluid dynamics we present a consistent new generalization of Clark and Putterman's equations to a set of superfluid equations parameterized by 14 dissipative parameters. The results of our gravitational calculation fit perfectly into this enlarged framework. In particular we compute all the dissipative constants for the gravitational superfluid.