Over-abundant gamma-like signals around Solar disk shadows by twin bent and smeared muon and electron pairs secondaries, versus rare local TeV gamma

Cosmic rays with energies of tens of TeV and above, skimming the Sun, could fragment into pions. The resulting gamma photons and muons, as well as subsequent electron pairs, will reach us in the form of gamma or electromagnetic air-showers, gamma-like air-showers on Earth. Their multiple presence may soon be observed and disentangled by the LHAASO telescope array

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Publication Details

Published
2025-09-23
DOI
https://doi.org/10.22323/1.501.1291
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
0.00

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article

Over-abundant gamma-like signals around Solar disk shadows by twin bent and smeared muon and electron pairs secondaries, versus rare local TeV gamma

O. Tibolla, Daniele Fargion, Danila O. Sopin, Pier Giorgio De Sanctis Lucentini et al.
Dark Matter and Cosmic Phenomena
article

Over-abundant gamma-like signals around Solar disk shadows by twin bent and smeared muon and electron pairs secondaries, versus rare local TeV gamma

O. Tibolla, Daniele Fargion, Danila O. Sopin, Pier Giorgio De Sanctis Lucentini, Maxim Khlopov, S. Kaufmann, S. Turriziani
article en

Abstract

Cosmic rays with energies of tens of TeV and above, skimming the Sun, could fragment into pions. The resulting gamma photons and muons, as well as subsequent electron pairs, will reach us in the form of gamma or electromagnetic air-showers, gamma-like air-showers on Earth. Their multiple presence may soon be observed and disentangled by the LHAASO telescope array

Ministry of Science and Higher Education of the Russian Federation, Southern Federal University
Openalex Percentile: Top 89%
Dark Matter and Cosmic Phenomena
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