Bose-Einstein condensation and muon production in ultra-high energy cosmic ray particle collisions
arXiv:2309.06411 · doi:10.1134/S1063778824700108
Abstract
Collisions of cosmic ray particles with ultra-high initial energies with nuclei in the atmosphere open a wide room for appearing of the novel dynamical features for multiparticle production processes. In particular, the pion-lasing behavior driven by Bose-Einstein condensation would result in the shift to larger multiplicities and, as consequence, could provide, in general, the enhanced yield of cosmic muons. In the present work the critical value of the space charged particle density for onset of Bose-Einstein condensation of the boson (pion) wave-packets into the same wave-packet state is estimated within the model with complete multiparticle symmetrization for the energy domain corresponded to the ultra-high energy cosmic rays (UHECR). Energy dependence of mean density of charged pions is evaluated for the cases of absent of the Bose-Einstein effects and for presence of laser-like behavior of pions. The possible influence of the Bose-Einstein condensation is discussed for the muon production in UHECR particle collisions with the atmosphere.
13 pages, 4 figures. 4th International symposium on cosmic rays and astrophysics (ISCRA2023). Moscow, Russia, June 27 - 29, 2023
References in corpus (9)
- Cosmic Rays from the Knee to the Highest Energies
- Report on Tests and Measurements of Hadronic Interaction Properties with Air Showers
- Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers
- Energy dependence of slope parameter in elastic nucleon-nucleon scattering
- Mass Composition of UHECRs from Distributions Recorded by the Pierre Auger and Telescope Array Observatories
- Geometry and space-time extent of pion emission region at FCC energies
- The spectra and composition of Ultra High Energy Cosmic Rays and the measurement of the proton-air cross section
- Top pair production at ultra-high energies
- Single top quark production at ultra-high energies