Impact of modified characteristics of hadronic interactions on cosmic-ray observables for proton and nuclear primaries

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F24%3A00598928" target="_blank" >RIV/68378271:_____/24:00598928 - isvavai.cz</a>

Výsledek na webu

<a href="https://pos.sissa.it/444/245/pdf" target="_blank" >https://pos.sissa.it/444/245/pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.444.0245" target="_blank" >10.22323/1.444.0245</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Impact of modified characteristics of hadronic interactions on cosmic-ray observables for proton and nuclear primaries

Popis výsledku v původním jazyce

Having implemented the option to make ad-hoc modifications of cross-section, multiplicity, and elasticity of hadronic interactions during the development of cosmic-ray showers into the CORSIKA simulation package in a consistent way for both primary protons and arbitrary nuclei, we can study the impact of these modifications on a variety of observables for different primaries. The modifications of the interactions are generic, without any reference to a specific mechanism. The ranges of parameters are only restricted by existing experimental data from accelerators and nuclear emulsions. The complete 3-dimensional view of the showers provided by CORSIKA allows us to study not only the depth of the maximum of the longitudinal development of the showers and total particle yield at the ground but also to see how the modifications impact the signal at different distances from the shower core and at different energy thresholds for the detection of secondary particles at the ground.

Název v anglickém jazyce

Impact of modified characteristics of hadronic interactions on cosmic-ray observables for proton and nuclear primaries

Popis výsledku anglicky

Having implemented the option to make ad-hoc modifications of cross-section, multiplicity, and elasticity of hadronic interactions during the development of cosmic-ray showers into the CORSIKA simulation package in a consistent way for both primary protons and arbitrary nuclei, we can study the impact of these modifications on a variety of observables for different primaries. The modifications of the interactions are generic, without any reference to a specific mechanism. The ranges of parameters are only restricted by existing experimental data from accelerators and nuclear emulsions. The complete 3-dimensional view of the showers provided by CORSIKA allows us to study not only the depth of the maximum of the longitudinal development of the showers and total particle yield at the ground but also to see how the modifications impact the signal at different distances from the shower core and at different energy thresholds for the detection of secondary particles at the ground.

Druh

D - Stať ve sborníku

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

<a href="/cs/project/GM21-02226M" target="_blank" >GM21-02226M: Zkoumání hadronických interakcí za možnostmi LHC pomocí spršek kosmického záření</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2024

Kód důvěrnosti údajů

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

Název statě ve sborníku

Proceedings of Science

ISBN

—

ISSN

1824-8039

e-ISSN

—

Počet stran výsledku

8

Strana od-do

245-252

Název nakladatele

Sissa Medilab srl

Místo vydání

Trieste

Místo konání akce

Nagoya

Datum konání akce

26. 7. 2023

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

—