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@inproceedings{66701,
author = {Tursunov, Arman and Homola, Piotr and Alvarez Castillo, David E. and Budnev, Nikolai and Gupta, Alok C. and Hnatyk, Bohdan and Kasztelan, Marcin and Kovacs, Peter and Łozowski, Bartosz and Medvedev, Mikhail V. and Mozgova, Alona and Niedźwiecki, Michał and Pawlik, Maciej and Rosas, Matías and Rzecki, Krzysztof and Smelcerz, Katarzyna and Smolek, Karel and Stasielak, Jarosław and Stuglik, Sławomir and Manana, Svanidze and Sushchov, Oleksandr and Verbetsky, Yuri and Wibig, Tadeusz and ZamoraandSaa, Jilberto},
address = {Itálie},
booktitle = {Proceedings of Science},
doi = {http://dx.doi.org/10.22323/1.395.0472},
keywords = {Black holes; Cosmology; Earth atmosphere; Energy transfer; Gravitation; Plasma jets;Cosmic strings; Cosmic-ray particles; Dark matter particles; Extra dimensions; Lorentz invariance violation; Relativistic plasmas; Ultra high-energy cosmic rays;CREDO},
howpublished = {elektronická verze "online"},
language = {eng},
location = {Itálie},
pages = {"472-1"-"472-5"},
publisher = {Sissa Medialab Srl},
title = {Probing UHECR and cosmic ray ensemble scenarios with a global CREDO network},
url = {https://pos.sissa.it/395/472},
year = {2022}
}
TY - JOUR
ID - 66701
AU - Tursunov, Arman - Homola, Piotr - Alvarez Castillo, David E. - Budnev, Nikolai - Gupta, Alok C. - Hnatyk, Bohdan - Kasztelan, Marcin - Kovacs, Peter - Łozowski, Bartosz - Medvedev, Mikhail V. - Mozgova, Alona - Niedźwiecki, Michał - Pawlik, Maciej - Rosas, Matías - Rzecki, Krzysztof - Smelcerz, Katarzyna - Smolek, Karel - Stasielak, Jarosław - Stuglik, Sławomir - Manana, Svanidze - Sushchov, Oleksandr - Verbetsky, Yuri - Wibig, Tadeusz - Zamora-Saa, Jilberto
PY - 2022
TI - Probing UHECR and cosmic ray ensemble scenarios with a global CREDO network
PB - Sissa Medialab Srl
CY - Itálie
KW - Black holes
KW - Cosmology
KW - Earth atmosphere
KW - Energy transfer
KW - Gravitation
KW - Plasma jets;Cosmic strings
KW - Cosmic-ray particles
KW - Dark matter particles
KW - Extra dimensions
KW - Lorentz invariance violation
KW - Relativistic plasmas
KW - Ultra high-energy cosmic rays;CREDO
UR - https://pos.sissa.it/395/472
N2 - Among theoretical approaches in unveiling the physics of ultra-high-energy cosmic rays (UHECR) one can distinguish the models assuming interactions of exotic super-heavy matter (including extra dimensions, Lorentz invariance violation, cosmic strings, dark matter particles or particles beyond the standard model etc.) and acceleration scenarios describing processes, in which the particles are accelerated by a particular astrophysical object (shocks in relativistic plasma jets, unipolar induction mechanisms, second-order Fermi acceleration, energy transfer from black holes or compact stars etc.). Primary UHECR particles can produce cascades already above the Earth atmosphere, which may be detected as the so-called cosmic ray ensembles (CRE) - the phenomena composed of at least two cosmic ray particles, including photons, with a common primary interaction vertex or the same parent particle with correlated arrival directions and arrival times. In this contribution, we give a brief description of a novel approach to the probing of cosmic ray scenarios with the global Cosmic Ray Extremely Distributed Observatory (CREDO) network.
ER -
TURSUNOV, Arman, Piotr HOMOLA, David E. ALVAREZ CASTILLO, Nikolai BUDNEV, Alok C. GUPTA, Bohdan HNATYK, Marcin KASZTELAN, Peter KOVACS, Bartosz ŁOZOWSKI, Mikhail V. MEDVEDEV, Alona MOZGOVA, Michał NIED$\backslash$'ZWIECKI, Maciej PAWLIK, Matías ROSAS, Krzysztof RZECKI, Katarzyna SMELCERZ, Karel SMOLEK, Jarosław STASIELAK, Sławomir STUGLIK, Svanidze MANANA, Oleksandr SUSHCHOV, Yuri VERBETSKY, Tadeusz WIBIG and Jilberto ZAMORA-SAA. Probing UHECR and cosmic ray ensemble scenarios with a global CREDO network. Online. In \textit{Proceedings of Science}. Itálie: Sissa Medialab Srl, 2022, p.~''472-1''-''472-5'', 5 pp. ISSN~1824-8039. Available from: https://dx.doi.org/10.22323/1.395.0472.
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