HOMOLA, Piotr, Dmitriy BEZNOSKO, Gopal BHATTA, Lukasz BIBRZYCKI, Michalina BORCZYNSKA, Lukasz BRATEK, Nikolay BUDNEV, Dariusz BURAKOWSKI, David E. ALVAREZ-CASTILLO, Kevin ALMEIDA CHEMINANT, Aleksander CWIKLA, Punsiri DAM-O, Niraj DHITAL, Alan R. DUFFY, Piotr GLOWNIA, Krzysztof GORZKIEWICZ, Dariusz GORA, Alok C. GUPTA, Zuzana HLAVKOVA, Martin HOMOLA, Joanna JALOCHA, Robert KAMINSKI, Michal KARBOWIAK, Marcin KASZTELAN, Renata KIEREPKO, Marek KNAP, Peter KOVACS, Szymon KULINSKI, Bartosz LOZOWSKI, Marek MAGRYS, Mikhail V. MEDVEDEV, Justyna MEDRALA, Jerzy W. MIETELSKI, Justyna MISZCZYK, Alona MOZGOVA, Antonio NAPOLITANO, Vahab NAZARI, Y. Jack NG, Michal NIEDZWIECKI, Cristina OANCEA, Boguslaw OGAN, Gabriela OPILA, Krzysztof OZIOMEK, Maciej PAWLIK, Marcin PIEKARCZYK, Boezna PONCYLJUSZ, Jerzy PRYGA, Matias ROSAS, Krzysztof RZECKI, Jilberto ZAMORA-SAA, Katarzyna SMELCERZ, Karel SMOLEK, Weronika STANEK, Jaroslaw STASIELAK, Slawomir STUGLIK, Jolanta SULMA, Oleksandr SUSHCHOV, Manana SVANIDZE, Kyle M. TAM, Arman TURSUNOV, Jose M. VAQUERO, Tadeusz WIBIG and Krzysztof W. WOZNIAK. Cosmic-Ray Extremely Distributed Observatory. Symmetry. 2020, vol. 12, No 11, p. "1835-1"-"1835-55", 55 pp. ISSN 2073-8994. Available from: https://dx.doi.org/10.3390/sym12111835.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name Cosmic-Ray Extremely Distributed Observatory
Authors HOMOLA, Piotr, Dmitriy BEZNOSKO, Gopal BHATTA, Lukasz BIBRZYCKI, Michalina BORCZYNSKA, Lukasz BRATEK, Nikolay BUDNEV, Dariusz BURAKOWSKI, David E. ALVAREZ-CASTILLO, Kevin ALMEIDA CHEMINANT, Aleksander CWIKLA, Punsiri DAM-O, Niraj DHITAL, Alan R. DUFFY, Piotr GLOWNIA, Krzysztof GORZKIEWICZ, Dariusz GORA, Alok C. GUPTA, Zuzana HLAVKOVA, Martin HOMOLA, Joanna JALOCHA, Robert KAMINSKI, Michal KARBOWIAK, Marcin KASZTELAN, Renata KIEREPKO, Marek KNAP, Peter KOVACS, Szymon KULINSKI, Bartosz LOZOWSKI, Marek MAGRYS, Mikhail V. MEDVEDEV, Justyna MEDRALA, Jerzy W. MIETELSKI, Justyna MISZCZYK, Alona MOZGOVA, Antonio NAPOLITANO, Vahab NAZARI, Y. Jack NG, Michal NIEDZWIECKI, Cristina OANCEA, Boguslaw OGAN, Gabriela OPILA, Krzysztof OZIOMEK, Maciej PAWLIK, Marcin PIEKARCZYK, Boezna PONCYLJUSZ, Jerzy PRYGA, Matias ROSAS, Krzysztof RZECKI, Jilberto ZAMORA-SAA, Katarzyna SMELCERZ, Karel SMOLEK, Weronika STANEK, Jaroslaw STASIELAK, Slawomir STUGLIK, Jolanta SULMA, Oleksandr SUSHCHOV, Manana SVANIDZE, Kyle M. TAM, Arman TURSUNOV (860 Uzbekistan, belonging to the institution), Jose M. VAQUERO, Tadeusz WIBIG and Krzysztof W. WOZNIAK.
Edition Symmetry, 2020, 2073-8994.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Switzerland
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/20:A0000060
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.3390/sym12111835
UT WoS 000593934200001
Keywords in English cosmic rays; cosmic-ray ensembles; extensive air showers; large scale cosmic-ray correlations; CREDO Collaboration
Tags , FÚ2020, RIV21
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 23/3/2021 21:28.
Abstract
The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a newly formed, global collaboration dedicated to observing and studying cosmic rays (CR) and cosmic-ray ensembles (CRE): groups of at least two CR with a common primary interaction vertex or the same parent particle. The CREDO program embraces testing known CR and CRE scenarios, and preparing to observe unexpected physics, it is also suitable for multi-messenger and multi-mission applications. Perfectly matched to CREDO capabilities, CRE could be formed both within classical models (e.g., as products of photon-photon interactions), and exotic scenarios (e.g., as results of decay of Super-Heavy Dark Matter particles). Their fronts might be significantly extended in space and time, and they might include cosmic rays of energies spanning the whole cosmic-ray energy spectrum, with a footprint composed of at least two extensive air showers with correlated arrival directions and arrival times. As the CRE are predominantly expected to be spread over large areas and, due to the expected wide energy range of the contributing particles, such a CRE detection might only be feasible when using all available cosmic-ray infrastructure collectively, i.e., as a globally extended network of detectors. Thus, with this review article, the CREDO Collaboration invites the astroparticle physics community to actively join or to contribute to the research dedicated to CRE and, in particular, to pool together cosmic-ray data to support specific CRE detection strategies.
PrintDisplayed: 6/5/2024 09:05