2022
Formation and propagation of cosmic-ray ensembles
SUSHCHOV, Oleksandr; Piotr HOMOLA; David E. ALVAREZ CASTILLO; Dmitriy BEZNOSKO; Nikolai BUDNEV et. al.Basic information
Original name
Formation and propagation of cosmic-ray ensembles
Authors
SUSHCHOV, Oleksandr; Piotr HOMOLA; David E. ALVAREZ CASTILLO; Dmitriy BEZNOSKO; Nikolai BUDNEV; Dariusz GÓRA; Alok C. GUPTA; Bohdan HNATYK; Marcin KASZTELAN; Peter KOVACS; Bartosz ŁOZOWSKI; Mikhail V. MEDVEDEV; Justyna MISZCZYK; Alona MOZGOVA; Vahab NAZARI; Michal NIEDŹWIECKI; Maciej PAWLIK; Matías ROSAS; Krzysztof RZECKI; Katarzyna SMELCERZ; Karel SMOLEK; Jaroslaw STASIELAK; Slawomir STUGLIK; Manana SVANIDZE; Arman TURSUNOV (860 Uzbekistan, belonging to the institution); Yuri VERBETSKY; Tadeusz WIBIG and Jilberto ZAMORA-SAA
Edition
Itálie, Proceedings of Science, p. "465-1"-"465-9", 9 pp. 2022
Publisher
Sissa Medialab Srl
Other information
Language
English
Type of outcome
Proceedings paper
Field of Study
10308 Astronomy
Country of publisher
Italy
Confidentiality degree
is not subject to a state or trade secret
Publication form
electronic version available online
References:
RIV identification code
RIV/47813059:19630/22:A0000241
Organization unit
Institute of physics in Opava
ISSN
EID Scopus
2-s2.0-85145258787
Keywords in English
Cosmology;Monte Carlo methods;Synchrotron radiation;Cosmic rays
Tags
International impact, Reviewed
Changed: 15/2/2023 15:36, Mgr. Pavlína Jalůvková
Abstract
In the original language
High-energy particles undergo different interactions while propagating through the Universe. As a result, they initiate particle cascades of various types and sizes, referred to as cosmic-ray ensembles (CRE). Since recently, Cosmic-Ray Extremely Distributed Observatory (CREDO) Collaboration aims at pursuing a mission dedicated to CRE, since this observation channel, i.e. correlated observation of cosmic rays on the global scale, complements the current approach to cosmic-ray research, which focuses on air showers initiated by individual cosmic rays. Recent results of Monte Carlo simulations showing that there might be a chance of observing a CRE originating from synchrotron radiation occurring even as far away from the Earth as at distances exceeding the Galaxy size, are presented. The issues and perspectives of the CRE-oriented research are discussed as well.