Pair condensation in a Finite Trapped Fermi Gas
arXiv:1210.4131 · doi:10.1103/PhysRevA.88.063643
Abstract
Superfluidity in the cold atomic two-species Fermi gas system in the unitary limit of infinite scattering length remains incompletely understood. In particular, a pseudogap phase has been proposed to exist above the superfluid critical temperature. Here we apply the auxiliary-field quantum Monte Carlo method to perform the first ab initio calculations of the temperature dependence of three quantities -- the energy-staggering pairing gap, the condensate fraction and the heat capacity -- in a trapped finite-size cold atom system. As the calculations of the energy-staggering pairing gap require the use of the canonical ensemble, we employ a novel algorithm for the stabilization of particle-number projection that is essential for reaching convergence in the size of the model space. We observe clear signatures of the superfluid phase transition in all three quantities, including a signature of the recently measured lambda peak in the heat capacity, but find no evidence of a pseudogap effect in the energy-staggering pairing gap.
5 pages, 1 figure. Added detail on stabilization method
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Cited by in corpus (10)
- Pairing of few Fermi atoms in one dimension
- Finite Temperature Auxiliary Field Quantum Monte Carlo in the Canonical Ensemble
- The contact in the unitary Fermi gas across the superfluid phase transition
- Pairing correlations across the superfluid phase transition in the unitary Fermi gas
- Emergence of a pseudogap in the BCS-BEC crossover
- The pseudogap regime in the unitary Fermi gas
- Calculating ground state properties of correlated fermionic systems with BCS trial wave functions in Slater determinant path-integral approaches
- Stabilizing Canonical-Ensemble Calculations in the Auxiliary-Field Monte Carlo Method
- A Stable, Recursive Auxiliary Field Quantum Monte Carlo Algorithm in the Canonical Ensemble: Applications to Thermometry and the Hubbard Model
- Structure Factors of The Unitary Gas Under Supernova Conditions