D 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

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.