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首页> 外文期刊>Theoretical and mathematical physics >INFLUENCE OF THE PSEUDOSCALAR CONDENSATE GRADIENT ON THE COOLING REGIME OF COMPACT STARS
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INFLUENCE OF THE PSEUDOSCALAR CONDENSATE GRADIENT ON THE COOLING REGIME OF COMPACT STARS

机译:伪张清氨酸凝结梯度对致密恒星冷却状态的影响

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摘要

We consider the processes in compact stars that arise during the potential formation of a pseudoscalar condensate in finite volumes. We do not propose specific hypotheses about the nature of this condensate. Considering that in the regions with a changing pseudoscalar density, photon propagation can be described in the framework of Maxwell-Chern-Simons electrodynamics, we find the reflection/transmission coefficients for regions with different densities. We study the fermion spectrum in the presence of an axial field considering the pseudoscalar condensate gradient. We also study the influence of the modified photon and fermion spectra on the cooling process of compact stars.
机译:我们考虑在有限体积中施加伪张清氨酸凝聚物的潜在形成期间出现的紧凑型恒星的过程。 我们不提出关于这种冷凝物的性质的具体假设。 考虑到在具有变化伪透视密度的区域中,可以在Maxwell-Chern-Simons电动力学的框架中描述光子传播,我们发现具有不同密度的区域的反射/传输系数。 考虑到伪影片凝胶梯度,我们在轴向场的存在下研究FERMION光谱。 我们还研究了改进的光子和FERMION光谱对紧凑型恒星冷却过程的影响。

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