Particle density fluctuations and correlations in low energy Cosmic-Ray showers simulated with CORSIKA

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19630%2F22%3AA0000240" target="_blank" >RIV/47813059:19630/22:A0000240 - isvavai.cz</a>

Alternative codes found

RIV/68407700:21670/22:00373818

Result on the web

<a href="https://pos.sissa.it/395/462" target="_blank" >https://pos.sissa.it/395/462</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.395.0462" target="_blank" >10.22323/1.395.0462</a>

Result language

angličtina

Original language name

Particle density fluctuations and correlations in low energy Cosmic-Ray showers simulated with CORSIKA

Original language description

The current studies of cosmic rays are focused on most energetic particles entering the atmosphere and producing a single Extensive Air Shower (EAS). There are, however, models predicting that interactions of high energy particles may result in Cosmic-Ray Ensembles (CRE) created far from the Earth. They could be observed as some number of correlated air showers of relatively low energies spread over a large area. The objective of the Cosmic Ray Extremely Distributed Observatory (CREDO) is to search for CRE using all available data from different detectors and observatories including even small but numerous detectors spread over large areas. Interpretation of such measurements require precise information on properties of EAS in a very wide energy spectrum. Low energy EAS are analysed using events from CORSIKA, the program performing air shower simulations. The primary cosmic ray particle energy range extends from 1 TeV up to 4 000 TeV. The secondary particles at the ground level are studied in order to obtain their density fluctuations and correlations in location. Although the fluctuations observed in multiplicity distributions are consistent with random the more detailed analysis reveals that near a selected particle the density of other particles is enhanced over that expected in the absence of correlations. The results of this analysis may be useful in further calculations, for example to obtain probability of detection of an EAS without special simulations.

Czech name

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Czech description

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Type

D - Article in proceedings

CEP classification

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OECD FORD branch

10308 - Astronomy (including astrophysics,space science)

Project

<a href="/en/project/EF16_019%2F0000766" target="_blank" >EF16_019/0000766: Engineering applications of microworld physics</a><br>

Continuities

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year

2022

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

Proceedings of Science

ISBN

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ISSN

1824-8039

e-ISSN

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Number of pages

8

Pages from-to

„462-1“-„462-8“

Publisher name

Sissa Medialab Srl

Place of publication

Itálie

Event location

Berlin

Event date

Jul 12, 2021

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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