ÚTEFČVUT Ústav technické a experimentální fyziky ČVUT v PrazeInstitute of Experimental and Applied Physics, CTU in Prague

Cosmic-Ray Extremely Distributed Observatory: Status and Perspectives

NázevTitle
Cosmic-Ray Extremely Distributed Observatory: Status and PerspectivesCosmic-Ray Extremely Distributed Observatory: Status and Perspectives
Druh výsledkuResult type
Článek v časopiseJournal article
AutořiAuthors
D. Gora, K. Cheminant, D. Alvarez-Castillo, L. Bratek, K. Smolek
Klíčová slovaKeywords
energy photon propagation, simulation
KonferenceConference
7th International Conference on New Frontiers in Physics (Kolymbari, Greece, 2018-07-04)
DOIDOI
10.3390/universe4110111
Časopis / citaceJournal / citation
Universe 4(11), 111 (2018) · ISSN 2218-1997
RokYear
2018
JazykLanguage
eng
ZáznamyRecords
ProjektProject
Inženýrské aplikace fyziky mikrosvětaEngineering applications of microworld physics
CitovánoCited by
12 (INSPIRE-HEP)
2019: 22020: 32021: 32022: 12023: 12024: 2
Plný text (open access)Full text (open access)
https://www.mdpi.com/2218-1997/4/11/111/pdf?version=1541643324
Citace ke staženíDownload citation
TXT · BibTeX

AbstraktAbstract

The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a project dedicated to global studies of extremely extended cosmic-ray phenomena, the cosmic-ray ensembles (CRE), beyond the capabilities of existing detectors and observatories. Up to date, cosmic-ray research has been focused on detecting single air showers, while the search for ensembles of cosmic-rays, which may overspread a significant fraction of the Earth, is a scientific terra incognita. Instead of developing and commissioning a completely new global detector infrastructure, CREDO proposes approaching the global cosmic-ray analysis objectives with all types of available detectors, from professional to pocket size, merged into a worldwide network. With such a network it is possible to search for evidences of correlated cosmic-ray ensembles. One of the observables that can be investigated in CREDO is a number of spatially isolated events collected in a small time window which could shed light on fundamental physics issues. The CREDO mission and strategy requires active engagement of a large number of participants, also non-experts, who will contribute to the project by using common electronic devices (e.g., smartphones). In this note, the status and perspectives of the project are presented.

The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a project dedicated to global studies of extremely extended cosmic-ray phenomena, the cosmic-ray ensembles (CRE), beyond the capabilities of existing detectors and observatories. Up to date, cosmic-ray research has been focused on detecting single air showers, while the search for ensembles of cosmic-rays, which may overspread a significant fraction of the Earth, is a scientific terra incognita. Instead of developing and commissioning a completely new global detector infrastructure, CREDO proposes approaching the global cosmic-ray analysis objectives with all types of available detectors, from professional to pocket size, merged into a worldwide network. With such a network it is possible to search for evidences of correlated cosmic-ray ensembles. One of the observables that can be investigated in CREDO is a number of spatially isolated events collected in a small time window which could shed light on fundamental physics issues. The CREDO mission and strategy requires active engagement of a large number of participants, also non-experts, who will contribute to the project by using common electronic devices (e.g., smartphones). In this note, the status and perspectives of the project are presented.

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