Finite temperature description of an interacting Bose gas

被引:8
作者
Sharma, Anushrut [1 ]
Kartvelishvili, Guram [1 ]
Khoury, Justin [1 ]
机构
[1] Univ Penn, Ctr Particle Cosmol, Dept Phys & Astron, Philadelphia, PA 19104 USA
关键词
TIME PHASE-TRANSITION; LINEAR SIGMA-MODEL; CHIRAL-SYMMETRY; LIQUID-HELIUM; GALACTIC HALO; SUPERFLUIDITY; DYNAMICS;
D O I
10.1103/PhysRevD.106.045025
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We derive the equation of state of a Bose gas with contact interactions using relativistic quantum field theory. The calculation accounts for both thermal and quantum corrections up to one-loop order. We work in the Hartree-Fock-Bogoliubov approximation and follow Yukalov's prescription of introducing two chemical potentials, one for the condensed phase and another one for the excited phase, to circumvent the well-known Hohenberg-Martin dilemma. As a check on the formalism, we take the nonrelativistic limit and reproduce the known results. Finally, we translate our results to the hydrodynamical, two-fluid model for finite-temperature superfluids. Our results are relevant for the phenomenology of Bose-Einstein condensate and superfluid dark matter candidates, as well as the color-flavor locking phase of quark matter in neutron stars.
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页数:15
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