大质量光子的概念及其天体物理学意义

G. A. Saiyan
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摘要

我们讨论了大质量光子的概念及其在天体物理学中可能产生的影响。我们使用了 "质量当量 "一词,而不是相对论质量或有效质量。我们还分析了修正的普朗克定律以及与大质量光子黑体辐射温度有关的估计(平均质量/剩余质量)比值。该比值在高温下发散,在低温下接近统一。据估计,CMB 辐射的 "质量当量 "相当于宇宙总质量的 0.0468%。我们讨论了早期宇宙中粒子-反粒子产生的布赖特-维勒过程的重要性。我们利用引力红移和宇宙学红移评估了光子静止质量的上限。我们发现光子的估计质量与用于估计质量的光谱波段的最低/最高频率之间存在相关性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The concept of the massive photon and its astrophysical implications
We discuss the concept of the massive photon with its possible implications in astrophysics. We use the term ”mass equivalent” instead of relativistic or effective mass. We also analyzed modified Planck’s law and estimated (mean mass/rest mass) ratio in connection to the temperature of blackbody radiation of the massive photons. This ratio diverges at high temperatures and approaches unity at low temperatures. The ”mass equivalent” for the CMB radiation was estimated to be equal to 0.0468% of the total mass of the Universe. We have discussed importance of the Breit-Wheeler process of particle – antiparticle production in the early Universe. We have evaluated the upper limit of the rest mass of the photon using gravitational and cosmological redshifts. A correlation was found between estimated masses of the photon and the lowest/highest frequencies of the spectral bands used for estimation of the mass.
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