About the possible signature of pion bose condensation contribution in the high energy cosmic ray nuclear interactions
T.T. Barnaveli, T.T. Barnaveli Jr, A.P. Chubenko, N.A. Eristavi, N.M., Nesterova, I.V. Khaldeeva

TL;DR
This paper investigates the potential signature of pion Bose condensation in high-energy cosmic ray interactions, suggesting it significantly influences anomalous energy deposit events observed in cosmic ray experiments.
Contribution
It provides evidence supporting the role of pion Bose condensation in high-energy nuclear interactions based on cosmic ray data analysis.
Findings
Evidence of pion Bose condensation contribution in cosmic ray interactions
Correlation between anomalous energy deposits and pion condensation signatures
Implications for nuclear matter in neutron stars and nuclei
Abstract
The events of anomalous energy deposit and high number of hadrons in hadron calorimeter, often not accompanied at all, or accompanied by very small EAS of cosmic rays, are observed by means of the complex installation aimed at research of cosmic rays. The data quoted and their analysis point to the real contribution and the essential role of pion Bose condensation in high energy nuclear interactions. The possibility of the existence of such process in the nuclear matter (in the neutron stars and in some kinds of the nuclei) was proposed by A.B.Migdal in 1971.
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Taxonomy
TopicsHigh-Energy Particle Collisions Research · Cosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena
