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, Yuri VERBETSKY, Tadeusz WIBIG and Jilberto ZAMORA-SAA. Formation and propagation of cosmic-ray ensembles. Online. In Proceedings of Science. Itálie: Sissa Medialab Srl, 2022, p. "465-1"-"465-9", 9 pp. ISSN 1824-8039. Available from: https://dx.doi.org/10.22323/1.395.0465.
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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
Original 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
WWW URL
RIV identification code RIV/47813059:19630/22:A0000241
Organization unit Institute of physics in Opava
ISSN 1824-8039
Doi http://dx.doi.org/10.22323/1.395.0465
Keywords in English Cosmology;Monte Carlo methods;Synchrotron radiation;Cosmic rays
Tags , RIV23
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 15/2/2023 15:36.
Abstract
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.
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