Condensation Energy of a Spin-1/2 Strongly Interacting Fermi Gas
arXiv:1304.1661 · doi:10.1103/PhysRevA.88.063614
Abstract
We report a measurement of the condensation energy of a two-component Fermi gas with tunable interactions. From the equation of state of the gas, we infer the properties of the normal phase in the zero-temperature limit. By comparing the pressure of the normal phase at T=0 to that of the low-temperature superfluid phase, we deduce the condensation energy, i.e. the energy gain of the system in being in the superfluid rather than normal state. We compare our measurements to a ladder approximation description of the normal phase, and to a fixed node Monte-Carlo approach, finding excellent agreement. We discuss the relationship between condensation energy and pairing gap in the BEC-BCS crossover.
4 figures
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Cited by in corpus (7)
- Ground-state thermodynamic quantities of homogeneous spin- fermions from the BCS region to the unitarity limit
- Phase structure of spin-imbalanced unitary Fermi gases
- Finite-temperature equation of state of polarized fermions at unitarity
- Direct Observation of Fragmentation in a Disordered, Strongly Interacting Fermi Gas
- Sarma phase in relativistic and non-relativistic systems
- Pairing patterns in polarized unitary Fermi gases above the superfluid transition
- SU(N) Fermi liquid at finite temperature