A New Method of Simulation of Cosmic-ray Ensembles Initiated by
Synchrotron Radiation

J 2022

A New Method of Simulation of Cosmic-ray Ensembles Initiated by Synchrotron Radiation

SUSHCHOV, Oleksandr, Piotr HOMOLA, Marcin PIEKARCZYK, Ophir RUIMI, Kevin Almeida CHEMINANT et. al.

Basic information

Original name

A New Method of Simulation of Cosmic-ray Ensembles Initiated by Synchrotron Radiation

Authors

Edition

SYMMETRY-BASEL, Švýcarsko, 2022, 2073-8994

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Country of publisher

Switzerland

Confidentiality degree

není předmětem státního či obchodního tajemství

References:

URL

RIV identification code

RIV/47813059:19630/22:A0000232

Organization unit

Institute of physics in Opava

DOI

http://dx.doi.org/10.3390/sym14101961

UT WoS

000873492600001

Keywords in English

cosmic rays; ultra-high energy photons; cosmic-ray ensembles; synchrotron radiation; CREDO Collaboration

Abstract

V originále

Cosmic rays interact with fields and background radiation as they propagate in space, producing particle cascades of various sizes, shapes and constituents. The potential observation of at least parts of such phenomena, referred to as cosmic-ray ensembles (CRE), from Earth would open a new channel of cosmic-ray investigation, since it might be a manifestation of fundamental symmetries of nature. Research dedicated to CRE is one of the main scientific objectives of the Cosmic-Ray Extremely Distributed Observatory (CREDO) Collaboration, and with this article we address one of the cornerstones of the relevant scientific program: the simulation method dedicated to CRE studies. Here we focus on CRE resulting from synchrotron radiation by high energy electrons as one of the most prevalent energy loss processes. Providing the example of simulation output analysis, we demonstrate the advantages of our approach as well as discuss the possibility of generalization of current research.

Citovat

SUSHCHOV, Oleksandr, Piotr HOMOLA, Marcin PIEKARCZYK, Ophir RUIMI, Kevin Almeida CHEMINANT, Olaf BAR, Lukasz BIBRZYCKI, Bohdan HNATYK, Peter KOVACS, Bartosz LOZOWSKI, Michal NIEDZWIECKI, Slawomir STUGLIK, Arman TURSUNOV and Tadeusz WIBIG. A New Method of Simulation of Cosmic-ray Ensembles Initiated by Synchrotron Radiation. SYMMETRY-BASEL. Švýcarsko, 2022, vol. 14, No 10, p. "1961-1"-"1961-11", 11 pp. ISSN 2073-8994. Available from: https://dx.doi.org/10.3390/sym14101961.

@article{66001,
   author = {Sushchov, Oleksandr and Homola, Piotr and Piekarczyk, Marcin and Ruimi, Ophir and Cheminant, Kevin Almeida and Bar, Olaf and Bibrzycki, Lukasz and Hnatyk, Bohdan and Kovacs, Peter and Lozowski, Bartosz and Niedzwiecki, Michal and Stuglik, Slawomir and Tursunov, Arman and Wibig, Tadeusz},
   article_location = {Švýcarsko},
   article_number = {10},
   doi = {http://dx.doi.org/10.3390/sym14101961},
   keywords = {cosmic rays; ultra-high energy photons; cosmic-ray ensembles; synchrotron radiation; CREDO Collaboration},
   language = {eng},
   issn = {2073-8994},
   journal = {SYMMETRY-BASEL},
   title = {A New Method of Simulation of Cosmic-ray Ensembles Initiated by Synchrotron Radiation},
   url = {https://www.mdpi.com/2073-8994/14/10/1961},
   volume = {14},
   year = {2022}
}

TY  - JOUR
ID  - 66001
AU  - Sushchov, Oleksandr - Homola, Piotr - Piekarczyk, Marcin - Ruimi, Ophir - Cheminant, Kevin Almeida - Bar, Olaf - Bibrzycki, Lukasz - Hnatyk, Bohdan - Kovacs, Peter - Lozowski, Bartosz - Niedzwiecki, Michal - Stuglik, Slawomir - Tursunov, Arman - Wibig, Tadeusz
PY  - 2022
TI  - A New Method of Simulation of Cosmic-ray Ensembles Initiated by Synchrotron Radiation
JF  - SYMMETRY-BASEL
VL  - 14
IS  - 10
SP  - "1961-1"-"1961-11"
EP  - "1961-1"-"1961-11"
SN  - 20738994
KW  - cosmic rays
KW  - ultra-high energy photons
KW  - cosmic-ray ensembles
KW  - synchrotron radiation
KW  - CREDO Collaboration
UR  - https://www.mdpi.com/2073-8994/14/10/1961
N2  - Cosmic rays interact with fields and background radiation as they propagate in space, producing particle cascades of various sizes, shapes and constituents. The potential observation of at least parts of such phenomena, referred to as cosmic-ray ensembles (CRE), from Earth would open a new channel of cosmic-ray investigation, since it might be a manifestation of fundamental symmetries of nature. Research dedicated to CRE is one of the main scientific objectives of the Cosmic-Ray Extremely Distributed Observatory (CREDO) Collaboration, and with this article we address one of the cornerstones of the relevant scientific program: the simulation method dedicated to CRE studies. Here we focus on CRE resulting from synchrotron radiation by high energy electrons as one of the most prevalent energy loss processes. Providing the example of simulation output analysis, we demonstrate the advantages of our approach as well as discuss the possibility of generalization of current research.
ER  -

SUSHCHOV, Oleksandr, Piotr HOMOLA, Marcin PIEKARCZYK, Ophir RUIMI, Kevin Almeida CHEMINANT, Olaf BAR, Lukasz BIBRZYCKI, Bohdan HNATYK, Peter KOVACS, Bartosz LOZOWSKI, Michal NIEDZWIECKI, Slawomir STUGLIK, Arman TURSUNOV and Tadeusz WIBIG. A New Method of Simulation of Cosmic-ray Ensembles Initiated by Synchrotron Radiation. \textit{SYMMETRY-BASEL}. Švýcarsko, 2022, vol.~14, No~10, p.~''1961-1''-''1961-11'', 11 pp. ISSN~2073-8994. Available from: https://dx.doi.org/10.3390/sym14101961.

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