Thermodynamics of Ideal Boson and Fermion Gases in the Static Taub Universe
Wung-Hong Huang

TL;DR
This paper investigates how small anisotropies in the curvature of a static Taub universe influence the thermodynamic properties of ideal boson and fermion gases, revealing configuration-dependent effects on condensation and particle distributions.
Contribution
It introduces a first-order analysis of thermodynamic quantities in an anisotropic universe and interprets these effects through a statistical interparticle potential framework.
Findings
Curvature anisotropy increases Bose-Einstein condensation in oblate universe.
Anisotropy decreases fermion distribution at low temperature.
Anisotropy enhances statistical attraction among bosons and repulsion among fermions.
Abstract
Some thermodynamic quantities of nonrelativistic ideal boson and fermion gases in the static Taub universe are derived to first order in a small anisotropy parameter d which measuring the deformation from the spherical Einstein universe. They are used to investigate the problem of how the curvature anisotropy affects the thermodynamic behaviors of an ideal gas. It is found that, when the universe is in the oblate configuration (i.e., d > 0), the effect of curvature anisotropy is to increase the number of the fraction in the Bose-Einstein condensation and to decrease the fermion distribution function at low temperature. When the universe is in the prolate configuration (i.e., d < 0), the effects of curvature anisotropy on the thermodynamic quantities is contrary to that in the oblate configuration. The density matrix of a two particle system is evaluated and it is used to define the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
