Abstract
We derive the underlying finite temperature theory which describes Fermi gas superfluidity with population imbalance in a homogeneous system. We compute the pair formation temperature, superfluid transition temperature , and superfluid density in a manner consistent with the standard ground state equations and, thereby, present a complete phase diagram. Finite temperature stabilizes superfluidity, as manifested by two solutions for or by low instabilities. At unitarity, the polarized state is an “intermediate-temperature superfluid.”
- Received 1 May 2006
DOI:https://doi.org/10.1103/PhysRevLett.97.090402
©2006 American Physical Society