HOMOLA, Piotr, David E. ALVAREZ CASTILLO, Kevin Almeida CHEMINANT, 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, Michał NIEDŹWIECKI, Maciej PAWLIK, Matías ROSAS, Krzysztof RZECKI, Katarzyna SMELCERZ, Karel SMOLEK, Jarosław STASIELAK, Sławomir STUGLIK, Oleksandr SUSHCHOV, Manana SVANIDZE, Arman TURSUNOV, Jose M. VAQUERO, Yuri VERBETSKY, Tadeusz WIBIG, Krzysztof WOŹNIAK a Jilberto ZAMORA-SAA. Invitation to the Cosmic Ray Extremely Distributed Observatory. Online. In Proceedings of Science. Itálie: Sissa Medialab Srl, 2022, s. "942-1"-"942-9", 9 s. ISSN 1824-8039. Dostupné z: https://dx.doi.org/10.22323/1.395.0942.
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Základní údaje
Originální název Invitation to the Cosmic Ray Extremely Distributed Observatory
Autoři HOMOLA, Piotr, David E. ALVAREZ CASTILLO, Kevin Almeida CHEMINANT, 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, Michał NIEDŹWIECKI, Maciej PAWLIK, Matías ROSAS, Krzysztof RZECKI, Katarzyna SMELCERZ, Karel SMOLEK, Jarosław STASIELAK, Sławomir STUGLIK, Oleksandr SUSHCHOV, Manana SVANIDZE, Arman TURSUNOV (860 Uzbekistán, domácí), Jose M. VAQUERO, Yuri VERBETSKY, Tadeusz WIBIG, Krzysztof WOŹNIAK a Jilberto ZAMORA-SAA.
Vydání Itálie, Proceedings of Science, od s. "942-1"-"942-9", 9 s. 2022.
Nakladatel Sissa Medialab Srl
Další údaje
Originální jazyk angličtina
Typ výsledku Stať ve sborníku
Obor 10308 Astronomy
Stát vydavatele Itálie
Utajení není předmětem státního či obchodního tajemství
Forma vydání elektronická verze "online"
WWW URL
Kód RIV RIV/47813059:19630/22:A0000243
Organizační jednotka Fyzikální ústav v Opavě
ISSN 1824-8039
Doi http://dx.doi.org/10.22323/1.395.0942
Klíčová slova anglicky Cosmology;Earth atmosphere;cosmic ray;Dark matter particles;
Štítky , RIV23
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnila: Mgr. Pavlína Jalůvková, učo 25213. Změněno: 15. 2. 2023 15:37.
Anotace
Cosmic Ray Ensembles (CRE) are very large, yet not observed particle cascades initiated above the Earth atmosphere. Such cascades could be formed both within classical models (e.g. products of photon-photon interactions) and exotic scenarios (e.g. result of decay of Super Heavy Dark Matter particles and subsequent interactions). Some of CRE might have a significant spatial extent which could serve as a unique signature detectable with the existing cosmic ray infrastructure taken as a network of detectors. This signature would be composed of a number of air showers with parallel axes. An obvious, although yet not probed, CRE „detection horizon” can be located somewhere between an air shower induced by an CRE composed of tightly collimated particles (preshower effect), and undetectable CRE composed of particles spread so widely that only one of them have a chance to reach Earth. Probing the CRE horizon with a global approach to the cosmic ray data, as proposed by the newly formed Cosmic Ray Extremely Distributed Observatory (CREDO), defines an extensive scientific program oriented on the search for physics manifestations at largest energies known, with potential impact on ultra-high energy astrophysics, the physics of fundamental particle interactions and cosmology. In this talk the current status and perspectives of CREDO will be summarized, with an open invitation for the colleagues interested in a global approach to cosmic ray studies, and in particular in observing and investigating multi-primary cosmic ray events such as CRE.
VytisknoutZobrazeno: 6. 5. 2024 21:53