D 2022

Determination of Zenith Angle Dependence of Incoherent Cosmic Ray Muon Flux Using Smartphones of the CREDO Project

WIBIG, Tadeusz, Michał KARBOWIAK, David ALVAREZ-CASTILLO, Olaf BAR, Łukasz BIBRZYCKI et. al.

Základní údaje

Originální název

Determination of Zenith Angle Dependence of Incoherent Cosmic Ray Muon Flux Using Smartphones of the CREDO Project

Autoři

WIBIG, Tadeusz, Michał KARBOWIAK, David ALVAREZ-CASTILLO, Olaf BAR, Łukasz BIBRZYCKI, Dariusz GORA, Piotr HOMOLA, Péter KOVÁCS, Marcin PIEKARCZYK, Jaroslaw STASIELAK, Sławomir STUGLIK, Oleksandr SUSHCHOV a Arman TURSUNOV (860 Uzbekistán, domácí)

Vydání

Itálie, Proceedings of Science, od s. "199-1"-"199-8", 8 s. 2022

Nakladatel

Sissa Medialab Srl

Další údaje

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"

Odkazy

Kód RIV

RIV/47813059:19630/22:A0000252

Organizační jednotka

Fyzikální ústav v Opavě

ISSN

Klíčová slova anglicky

CREDO project;Cosmic ray detectors; Cosmology; Smartphones;Charged particles;Cosmic-ray particles; Extensive air showers; Muon flux; Shower array; Smart phones; Ultra high-energy cosmic rays; Zenith angle

Štítky

Příznaky

Mezinárodní význam, Recenzováno
Změněno: 16. 2. 2023 13:25, Mgr. Pavlína Jalůvková

Anotace

V originále

The Cosmic-Ray Extremely Distributed Observatory (CREDO) was established to detect and study ultra high-energy cosmic ray particles. In addition to making use of traditional methods for finding rare and extended cosmic ray events such as professional-grade Extensive Air Shower (EAS) arrays, as well as educational 'class-room' detectors, CREDO also makes use of cameras in smartphones as particle detectors. Beyond the primary scientific goal of the CREDO project, to detect Cosmic Ray Ensembles, is the equally important educational goal of the project. To use smartphones for EAS detection, it is necessary to demonstrate that they are capable of effectively registering relativistic charged particles. In this article we show that the events recorded in the CREDO project database are indeed tracing incoherent cosmic ray muons. The specific observed distribution of the zenith angle of the charged particle direction corresponds to that expected for muons. It is difficult, if not impossible, to imagine the different mechanisms leading to such a distribution, and we believe it clearly demonstrates the suitability of smartphone-based detectors in supporting the more traditional cosmic ray detectors.