Thermal Casimir effect for a Dirac field on flat space with a nontrivial circular boundary condition

Fuente: arXiv
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Main Authors: Venâncio, Joás, Filho, Lameque, Mota, Herondy, Mohammadi, Azadeh
Format: Preprint
Published: 2024
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author Venâncio, Joás
Filho, Lameque
Mota, Herondy
Mohammadi, Azadeh
author_facet Venâncio, Joás
Filho, Lameque
Mota, Herondy
Mohammadi, Azadeh
contents This work investigates the thermal Casimir effect associated with a massive spinor field defined on a four-dimensional flat space with a circularly compactified spatial dimension whose periodicity is oriented along a vector in $xy$-plane. We employ the generalized zeta function method to establish a finite definition for the vacuum free energy density. This definition conveniently separates into the zero-temperature Casimir energy density and additional terms accounting for temperature corrections. The structure of existing divergences is analyzed from the asymptotic behavior of the spinor heat kernel function and removed in the renormalization by subtracting scheme. The only non-null heat coefficient is the one associated with the Euclidean divergence. We also address the need for a finite renormalization to treat the ambiguity in the zeta function regularization prescription \text{associated} with this Euclidean heat kernel coefficient and ensure that the renormalization procedure is unique. The high- and low-temperature asymptotic limits are also explored. In particular, we explicitly show that free energy density lacks a classical limit at high temperatures, and the entropy density agrees with the Nernst heat theorem at low temperatures.
format Preprint
id arxiv_https___arxiv_org_abs_2404_05918
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Thermal Casimir effect for a Dirac field on flat space with a nontrivial circular boundary condition
Venâncio, Joás
Filho, Lameque
Mota, Herondy
Mohammadi, Azadeh
High Energy Physics - Theory
This work investigates the thermal Casimir effect associated with a massive spinor field defined on a four-dimensional flat space with a circularly compactified spatial dimension whose periodicity is oriented along a vector in $xy$-plane. We employ the generalized zeta function method to establish a finite definition for the vacuum free energy density. This definition conveniently separates into the zero-temperature Casimir energy density and additional terms accounting for temperature corrections. The structure of existing divergences is analyzed from the asymptotic behavior of the spinor heat kernel function and removed in the renormalization by subtracting scheme. The only non-null heat coefficient is the one associated with the Euclidean divergence. We also address the need for a finite renormalization to treat the ambiguity in the zeta function regularization prescription \text{associated} with this Euclidean heat kernel coefficient and ensure that the renormalization procedure is unique. The high- and low-temperature asymptotic limits are also explored. In particular, we explicitly show that free energy density lacks a classical limit at high temperatures, and the entropy density agrees with the Nernst heat theorem at low temperatures.
title Thermal Casimir effect for a Dirac field on flat space with a nontrivial circular boundary condition
topic High Energy Physics - Theory
url https://arxiv.org/abs/2404.05918