发表机构
Lebedev Physical Institute, Russian Academy of Sciences; Moscow Aviation Institute (National Research University)（列别捷夫物理研究所，俄罗斯科学院; 莫斯科航空学院（国立研究大学））
机构由 AI 辅助整理，请以论文原文为准。AI 中文总结
本文提出局域源光子场模型，解释宇宙线能谱中100 PeV附近“隆起”的形成，认为该特征源于刍藁型变星（红巨星与白矮星系统）对初级宇宙辐射的影响。
AI 中文摘要
本文研究了局域源（LS）的光子场对宇宙线（CR）能谱（E0）形成的影响。基于局域源模型，提出了宇宙线能谱中不规则性形成的模型。研究表明，宇宙线能谱可以表示为局部宇宙线源附近初级宇宙辐射（PCR）穿过源的光子场时形成的部分谱之和。局域源可以是恒星种群中各种变星类型中最活跃的恒星，从矮星到超巨星。研究显示，在刍藁型变星的光子场中，在E0 = 100 PeV附近形成了所谓的“隆起”，这类变星通常是包含红巨星和白矮星的多星系统。
英文摘要
The influence of photon fields of local sources (LS) on the formation of the cosmic ray (CR) energy spectrum (E0) is considered. A model for the formation of irregularities in the CR spectrum, based on the local source model, is proposed. It is shown that the CR spectrum can be formed as a sum of partial spectra formed near local CR sources during the passage of primary cosmic radiation (PCR) through the photon fields of the sources. Local sources can be the most active stars of various types of variability in the stellar population, - from dwarfs to hypergiants. Studies have shown that the so-called "bump" near E0 = 100 PeV is formed in the photon fields of Mira-type variable stars, which are typically multiple stellar systems, consisting of a red giant and a white dwarf.
