轴向相互作用诱发的费米子凝聚态及其宇宙学意义

IF 4.3 3区 材料科学 Q1 ENGINEERING, ELECTRICAL & ELECTRONIC
A Capolupo, A Quaranta
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引用次数: 0

摘要

我们揭示了由自旋-自旋相互作用产生的凝聚真空所导致的轴电流的新来源。为了证明这一点,我们考虑了一个包含自旋-自旋相互作用项的四元狄拉克拉格朗日,它可能源于爱因斯坦-卡坦类理论中的扭转。我们使用均值场方法来分析量子化理论。我们证明,场哈密顿的对角化定义了一种新的真空状态,相对于自由真空而言,它在能量上更有利。这种真空是粒子对-反粒子对的凝聚态,其特征是轴流算子的期望值并非微不足道。根据自旋-自旋相互作用项的起源,这里获得的新轴流源可以在原子层面和天体物理学-宇宙学层面产生影响。凝聚态自发地打破了洛伦兹对称性,因此它意味着早期宇宙中存在违反 CPT 的可能性。此外,凝聚态还在引力场方程中诱发了一个新的源项,并可能在宇宙学层面上影响宇宙的暗部。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Fermion condensates induced by axial interactions and cosmological implications
We reveal the presence of a new source of axial current due to the condensed vacuum generated by the spin–spin interaction. To show this, we consider a quartic Dirac Lagrangian containing a spin–spin interaction term, possibly originating from torsion in Einstein–Cartan-like theories. We use a mean field approach to analyze the quantized theory. We show that the diagonalization of the field Hamiltonian defines a new vacuum state, energetically favored with respect to the free vacuum. Such a vacuum, which is a condensate of particle-antiparticle pairs, is characterized by a nontrivial expectation value of the axial current operator. The new source of axial current, here obtained, can have effects both at the atomic level and at the astrophysical–cosmological level depending on the origin of the spin–spin interaction term. The condensate spontaneously breaks Lorentz symmetry, therefore it implies the possibility of CPT violation in the early universe. Furthermore the condensate induces a new source term in the gravitational field equations and may affect the dark sector of the Universe at cosmological level.
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来源期刊
CiteScore
7.20
自引率
4.30%
发文量
567
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