Detailed Information on Publication Record
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
Stať ve sborníku
Field of Study
10308 Astronomy
Country of publisher
Italy
Confidentiality degree
není předmětem státního či obchodního tajemství
Publication form
electronic version available online
References:
RIV identification code
RIV/47813059:19630/22:A0000241
Organization unit
Institute of physics in Opava
ISSN
Keywords in English
Cosmology;Monte Carlo methods;Synchrotron radiation;Cosmic rays
Tags
International impact, Reviewed
Změněno: 15/2/2023 15:36, Mgr. Pavlína Jalůvková
Abstract
V originále
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.