Towards a Non-Relativistic Holographic Superfluid
arXiv:1103.3472 · doi:10.1088/1367-2630/13/11/115008
Abstract
We explore the phase structure of a holographic toy model of superfluid states in non-relativistic conformal field theories. At low background mass density, we find a familiar second-order transition to a superfluid phase at finite temperature. Increasing the chemical potential for the probe charge density drives this transition strongly first order as the low-temperature superfluid phase merges with a thermodynamically disfavored high-temperature condensed phase. At high background mass density, the system reenters the normal phase as the temperature is lowered further, hinting at a zero-temperature quantum phase transition as the background density is varied. Given the unusual thermodynamics of the background black hole, however, it seems likely that the true ground state is another configuration altogether.
13+5 pages, latex
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- Non-Relativistic Holography -- A Group-Theoretical Perspective
- Schrodinger Fermi Liquids
- Holographic charge diffusion in non relativistic branes
- The Godel-Schrodinger Spacetime and Stringy Chronology Protection
- Exciton-driven quantum phase transitions in holography
- On S-duality for holographic p-wave superconductors