Cosmic-ray extremely distributed observatory

Homola P., Beznosko D., Bhatta G., Bibrzycki Ł., Borczyńska M., Bratek Ł., Budnev N., Burakowski D., Alvarez-Castillo D.E., Cheminant K.A., Ćwikła A., Dam-O P., Dhital N., Duffy A.R., Głownia P., Gorzkiewicz K., Góra D., Gupta A.C., Hlávková Z., Homola M., Jałocha J., Kamiński R., Karbowiak M., Kasztelan M., Kierepko R., Knap M., Kovács P., Kuliński S., Łozowski B., Magryś M., Medvedev M.V., Mędrala J., Mietelski J.W., Miszczyk J., Mozgova A., Napolitano A., Nazari V., Ng Y.J., Niedźwiecki M., Oancea C., Ogan B., Opiła G., Oziomek K., Pawlik M., Piekarczyk M., Poncyljusz B., Pryga J., Rosas M., Rzecki K., Zamora-Saa J., Smelcerz K., Smolek K., Stanek W., Stasielak J., Stuglik S., Sulma J., Sushchov O., Svanidze M., Tam K.M., Tursunov A., Vaquero J.M., Wibig T., Woźniak K.W.

Cosmic-ray extremely distributed observatory

Archivos

TEXTO COMPLETO EN INGLÉS

Fecha

2020-11

Autores

Homola P., Beznosko D., Bhatta G., Bibrzycki Ł., Borczyńska M., Bratek Ł., Budnev N., Burakowski D., Alvarez-Castillo D.E., Cheminant K.A., Ćwikła A., Dam-O P., Dhital N., Duffy A.R., Głownia P., Gorzkiewicz K., Góra D., Gupta A.C., Hlávková Z., Homola M., Jałocha J., Kamiński R., Karbowiak M., Kasztelan M., Kierepko R., Knap M., Kovács P., Kuliński S., Łozowski B., Magryś M., Medvedev M.V., Mędrala J., Mietelski J.W., Miszczyk J., Mozgova A., Napolitano A., Nazari V., Ng Y.J., Niedźwiecki M., Oancea C., Ogan B., Opiła G., Oziomek K., Pawlik M., Piekarczyk M., Poncyljusz B., Pryga J., Rosas M., Rzecki K., Zamora-Saa J., Smelcerz K., Smolek K., Stanek W., Stasielak J., Stuglik S., Sulma J., Sushchov O., Svanidze M., Tam K.M., Tursunov A., Vaquero J.M., Wibig T., Woźniak K.W.

Idioma

en

Editor

MDPI AG

Resumen

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. © 2020, MDPI AG. All rights reserved.

Notas

Indexación Scopus

Palabras clave

Extensive Air Showers, Cosmic Ray Showers, Neutrinos

Citación

Symmetry, Volume 12, Issue 11, Pages 1 - 55November 2020 Article number 1835

DOI

10.3390/sym12111835

URI

http://repositorio.unab.cl/xmlui/handle/ria/20744

Colecciones

FCE - Artículos de Revista

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