Sibyll*

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A90232%2F24%3A00641917" target="_blank" >RIV/68378271:90232/24:00641917 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1016/j.astropartphys.2024.102964" target="_blank" >https://doi.org/10.1016/j.astropartphys.2024.102964</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.astropartphys.2024.102964" target="_blank" >10.1016/j.astropartphys.2024.102964</a>

Result language
angličtina
Original language name
Sibyll*
Original language description
In the last decade, an increasing number of datasets have revealed a consistent discrepancy between the number of muons measured in ultrahigh-energy extensive air showers (EAS) and the numbers predicted by simulations. This gap persists despite incorporating Large Hadron Collider (LHC) data into the tuning of current hadronic interaction models, leading to the phenomenon often termed the 'muon puzzle'. To gain a deeper understanding of the potential origins of this muon puzzle, we have developed Sibyll* , a series of phenomenologically modified versions of Sibyll 2.3d. In these models, we have increased muon production by altering p(0) , baryon-antibaryon pair, or kaon production in hadronic multiparticle production processes.
Czech name
—
Czech description
—

Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
—
OECD FORD branch
10303 - Particles and field physics

Publication year
2024
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Similar results(10)