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The gluon condensation effect in the cosmic hadron spectra - MaRDI portal

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The gluon condensation effect in the cosmic hadron spectra

From MaRDI portal
Publication:5070930

DOI10.1088/1475-7516/2020/09/011zbMATH Open1493.85007arXiv2002.06294OpenAlexW3083433100MaRDI QIDQ5070930

Author name not available (Why is that?)

Publication date: 14 April 2022

Published in: (Search for Journal in Brave)

Abstract: Hardening of cosmic proton- and nuclei-spectra is explained by using the gluon condensation (GC) model, which states that a large amount of gluons in proton may condense near the high energy threshold. The results present the GC-effect as common origin of a series of anomalous astrophysical phenomena including the broken power-law in gamma-ray spectra, the excess in positron- and electron-spectra and hardening of proton- and nuclei-spectra.


Full work available at URL: https://arxiv.org/abs/2002.06294



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