Sound modes in holographic superfluids
Christopher P. Herzog, Amos Yarom
TL;DR
This work analyzes sound modes in a strongly interacting relativistic superfluid using a holographic AdS/CFT dual with a Maxwell field and a charged scalar in AdS$_5$. Through relativistic two-fluid hydrodynamics and a fully backreacted gravity model, it computes first, second, and fourth sound as functions of temperature, revealing that second sound at low $T$ does not conform to Landau's nonrelativistic incompressible limit. A key finding is the existence of a critical scalar charge $q_c(u)$ that governs the qualitative behavior of the sound modes, with monotonic second- and fourth-sound behavior emerging only above it. The results highlight substantial deviations from naive Landau theory in relativistic, strongly coupled holographic superfluids and illuminate the role of backreaction, thermodynamics, and quasi-particle dynamics in determining collective modes.
Abstract
Superfluids support many different types of sound waves. We investigate the relation between the sound waves in a relativistic and a non-relativistic superfluid by using hydrodynamics to calculate the various sound speeds. Then, using a particular holographic scalar gravity realization of a strongly interacting superfluid, we compute first, second and fourth sound speeds as a function of the temperature. The relativistic low temperature results for second sound differ from Landau's well known prediction for the non-relativistic, incompressible case.
