斯托纳相变热特性的惯性计算

IF 0.9 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY Acta Physica Polonica B Pub Date : 2023-09-26 DOI:10.5506/aphyspolb.54.11-a4
Oskar Grocholski, P. Chankowski
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引用次数: 0

摘要

我们将热(虚时)微扰展开应用于相关的有效场理论,计算了(非相对论)自旋 1/2 费米子通过短程自旋独立斥力二元相互作用势相互作用的气体在低温下向有序态相变的特征。我们展示了如何根据自旋上升和自旋下降费米子的密度 $n_+$ 和 $n_-$,获得系统自由能的系统扩展。在本文中,我们在二阶截断了这一扩展,并通过数值自由能最小化,确定了作为温度、系统总密度 $n = n_+ + n_-$ 和相互作用强度函数的 $n_+$ 和 $n_-$ 的平衡比例(即系统的极化)。
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Perturbative Computation of Thermal Characteristics of the Stoner Phase Transition
We apply the thermal (imaginary time) perturbative expansion to the relevant effective field theory to compute characteristics of the phase transition to the ordered state which can occur at low temperatures in the gas of (nonrelativistic) spin 1/2 fermions interacting through a short-range spin independent repulsive binary interaction potential. We show how to obtain a systematic expansion of the system's free energy depending on the densities $n_+$ and $n_-$ of spin-up and spin-down fermions. In this paper we truncate this expansion at the second order and determine, by numerically minimizing the free energy, the equilibrium proportions of $n_+$ and $n_-$ (that is, the system's polarization) as functions of the temperature, the system's overall density $n = n_+ + n_-$ and the strength of the interaction.
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来源期刊
Acta Physica Polonica B
Acta Physica Polonica B 物理-物理:综合
CiteScore
1.70
自引率
20.00%
发文量
30
审稿时长
3-8 weeks
期刊介绍: Acta Physica Polonica B covers the following areas of physics: -General and Mathematical Physics- Particle Physics and Field Theory- Nuclear Physics- Theory of Relativity and Astrophysics- Statistical Physics
期刊最新文献
Particle-theory Input for Neutron-star Physics Perturbative Computation of Thermal Characteristics of the Stoner Phase Transition Topologically Charged Rotating Wormhole The Mass Density Contrast in Perturbed Friedman–Lemaître–Robertson–Walker Cosmologies Wigner and Husimi Partonic Distributions of the Pion in a Chiral Quark Model
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