Simple and less hadronic-model-dependent method for cosmic-ray composition determination

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A90232%2F24%3A00604989" target="_blank" >RIV/68378271:90232/24:00604989 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1103/PhysRevD.109.043003" target="_blank" >https://doi.org/10.1103/PhysRevD.109.043003</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1103/PhysRevD.109.043003" target="_blank" >10.1103/PhysRevD.109.043003</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Simple and less hadronic-model-dependent method for cosmic-ray composition determination

Popis výsledku v původním jazyce

The origin and nature of ultrahigh-energy cosmic rays remains a mystery despite the great progress that has been made in recent years mainly due to the observations performed by the Pierre Auger Observatory and Telescope Array. In particular, the composition information of the cosmic rays as a function of the energy appears to be crucial for the understanding of their origin. The best observables for primary mass composition are the muon content of extensive air showers and the atmospheric depth of the shower maximum development. In this work we present a novel method which allows us to use any type of classification method to perform mass composition analyses based on the number of muons.n

Název v anglickém jazyce

Simple and less hadronic-model-dependent method for cosmic-ray composition determination

Popis výsledku anglicky

The origin and nature of ultrahigh-energy cosmic rays remains a mystery despite the great progress that has been made in recent years mainly due to the observations performed by the Pierre Auger Observatory and Telescope Array. In particular, the composition information of the cosmic rays as a function of the energy appears to be crucial for the understanding of their origin. The best observables for primary mass composition are the muon content of extensive air showers and the atmospheric depth of the shower maximum development. In this work we present a novel method which allows us to use any type of classification method to perform mass composition analyses based on the number of muons.n

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2024

Kód důvěrnosti údajů

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

Název periodika

Physical Review D

ISSN

2470-0010

e-ISSN

2470-0029

Svazek periodika

109

Číslo periodika v rámci svazku

4

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

11

Strana od-do

043003

Kód UT WoS článku

001175461700013

EID výsledku v databázi Scopus

2-s2.0-85184879890