Studying the mass sensitivity of air-shower observables using simulated cosmic rays

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A90232%2F24%3A00604970" target="_blank" >RIV/68378271:90232/24:00604970 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1103/PhysRevD.109.042002" target="_blank" >https://doi.org/10.1103/PhysRevD.109.042002</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1103/PhysRevD.109.042002" target="_blank" >10.1103/PhysRevD.109.042002</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Studying the mass sensitivity of air-shower observables using simulated cosmic rays

Popis výsledku v původním jazyce

Using CORSIKA simulations, we investigate the mass sensitivity of cosmic-ray air-shower observables for sites at the South Pole and Malargüe, Argentina, the respective locations of the IceCube Neutrino Observatory and the Pierre Auger Observatory. Exact knowledge of observables from air-shower simulations was used to study the event-by-event mass separation between proton, helium, oxygen, and iron primary cosmic rays with a Fisher linear discriminant analysis. Dependencies on the observation site as well as the energy and zenith angle of the primary particle were studied in the ranges from 10 16.0–10 18.5 eV and 0° to 60°, they are mostly weak and do not change the qualitative results.

Název v anglickém jazyce

Studying the mass sensitivity of air-shower observables using simulated cosmic rays

Popis výsledku anglicky

Using CORSIKA simulations, we investigate the mass sensitivity of cosmic-ray air-shower observables for sites at the South Pole and Malargüe, Argentina, the respective locations of the IceCube Neutrino Observatory and the Pierre Auger Observatory. Exact knowledge of observables from air-shower simulations was used to study the event-by-event mass separation between proton, helium, oxygen, and iron primary cosmic rays with a Fisher linear discriminant analysis. Dependencies on the observation site as well as the energy and zenith angle of the primary particle were studied in the ranges from 10 16.0–10 18.5 eV and 0° to 60°, they are mostly weak and do not change the qualitative results.

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

21

Strana od-do

042002

Kód UT WoS článku

001174872400006

EID výsledku v databázi Scopus

2-s2.0-85187279538