Szczegóły publikacji
Opis bibliograficzny
Cosmic-ray extremely distributed observatory / Piotr Homola, Dmitriy Beznosko, Gopal Bhatta, Łukasz Bibrzycki, Michalina Borczyńska, Łukasz Bratek, Nikolay Budnev, Dariusz Burakowski, David E. Alvarez-Castillo, Kevin Almeida Cheminant, Aleksander Ćwikła, Punsiri Dam-o, Niraj Dhital, Alan R. Duffy, Piotr Głownia, Krzysztof Gorzkiewicz, Dariusz Góra, Alok C. Gupta, Zuzana Hlávková, Martin Homola, Joanna Jałocha, Robert Kamiński, Michał Karbowiak, Marcin Kasztelan, Renata Kierepko, Marek Knap, Péter Kovács, Szymon Kuliński, Bartosz Łozowski, Marek MAGRYŚ, Mikhail V. Medvedev, Justyna Mędrala, Jerzy W. Mietelski, Justyna Miszczyk, Alona Mozgova, Antonio Napolitano, Vahab Nazari, Y. Jack Ng, Michał Niedźwiecki, Cristina Oancea, Bogusław Ogan, Gabriela Opiła, Krzysztof OZIOMEK, Maciej PAWLIK, Marcin Piekarczyk, Bożena Poncyljusz, Jerzy Pryga, Matías Rosas, Krzysztof RZECKI, Jilberto Zamora-Saa, Katarzyna Smelcerz, Karel Smolek, Weronika Stanek, Jarosław Stasielak, Sławomir Stuglik, Jolanta Sulma, Oleksandr Sushchov, Manana Svanidze, Kyle M. Tam, Arman Tursunov, José M. Vaquero, Tadeusz Wibig, Krzysztof W. Woźniak // Symmetry [Dokument elektroniczny]. — Czasopismo elektroniczne ; ISSN 2073-8994. — 2020 — vol. 12 iss. 11 art. no. 1835, s. 1–55. — Wymagania systemowe: Adobe Reader. — Bibliogr. s. 44–55, Abstr. — Publikacja dostępna online od: 2020-11-05
Autorzy (63)
- AGHMagryś Marek
- AGHMędrala Justyna
- AGHOpiła Gabriela
- AGHOziomek Krzysztof
- AGHPawlik Maciej
- AGHRzecki Krzysztof
- AGHStanek Weronika
- Almeida Cheminant Kevin
- Alvarez-Castillo David E.
- Beznosko Dmitriy
- Bhatta Gopal
- Bibrzycki Łukasz
- Borczyńska Michalina
- Bratek Łukasz
- Budnev Nikolay
- Burakowski Dariusz
- Ćwikła Aleksander
- Dam-o Punsiri
- Dhital Niraj
- Duffy Alan R.
- Głownia Piotr
- Gorzkiewicz Krzysztof
- Góra Dariusz
- Gupta Alok Chandra
- Hlávková Zuzana
- Homola Martin
- Homola Piotr
- Jałocha Joanna
- Kamiński Robert
- Karbowiak Michał
- Kasztelan Marcin
- Kierepko Renata
- Knap Marek
- Kovács Péter
- Kuliński Szymon
- Łozowski Bartosz
- Medvedev Mikhail V.
- Mietelski Jerzy W.
- Miszczyk Justyna
- Mozgova Alona
- Napolitano Antonio
- Nazari Vahab
- Ng Y. Jack
- Niedźwiecki Michał
- Oancea Cristina
- Ogan Bogusław
- Piekarczyk Marcin
- Poncyliusz Bożena
- Pryga Jerzy
- Rosas Matías
- Smelcerz Katarzyna
- Smolek Karel
- Stasielak Jarosław
- Stuglik Sławomir
- Sulma Jolanta
- Sushchov Oleksandr
- Svanidze Manana
- Tam Kyle M.
- Tursunov Arman
- Vaquero José M.
- Wibig Tadeusz
- Woźniak Krzysztof
- Zamora-Saa Jilberto
Słowa kluczowe
Dane bibliometryczne
| ID BaDAP | 130982 |
|---|---|
| Data dodania do BaDAP | 2020-11-09 |
| Tekst źródłowy | URL |
| DOI | 10.3390/sym12111835 |
| Rok publikacji | 2020 |
| Typ publikacji | artykuł w czasopiśmie |
| Otwarty dostęp |  |
| Creative Commons | |
| Czasopismo/seria | Symmetry |
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.
