Published 2019 | Version v1
Journal article

The hadronic interaction model Sibyll 2.3c and muon production in extensive air-showers

  • 1. Laboratório de Instrumentação e Física Experimental de Partículas (LIP), Av. Prof. Gama Pinto 2, 1649-003 Lisbon (Portugal)
  • 2. Karlsruher Institut für Technologie, Institut für Kernphysik, Postfach 3640, 76021 Karlsruhe (Germany)
  • 3. DESY, Platanenallee 6, 15738 Zeuthen (Germany)
  • 4. Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark, DE 19716 (US)

Description

One of the applications of the hadronic interaction model Sibyll is the simulation of extensive air showers of ultra-high energy cosmic rays. In recent years it has become more and more clear that simulations do not agree with measurements when it comes to observables related to muons in air showers. We discuss the processes in Sibyll that are directly related to muon production in extensive air showers and describe their relation to shower observables.

Availability note (English)

Available from https://www.epj-conferences.org/articles/epjconf/pdf/2019/13/epjconf_isvhecri2018_11002.pdf; https://doaj.org/article/cf6797eaad3a4dadbbf9136b7e9e5d1c

Additional details

Publishing Information

Journal Title
EPJ. Web of Conferences
Journal Volume
208
Journal Page Range
vp.
ISSN
2100-014X

Conference

Title
30. International Symposium on Very High Energy Cosmic Ray Interactions
Acronym
ISVHECRI 2018
Dates
21-25 May 2018
Place
Nagoya (Japan)

INIS

Country of Publication
France
Country of Input or Organization
France
INIS RN
53098373
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COMPUTERIZED SIMULATION; EXTENSIVE AIR SHOWERS; HADRONS; MUONS; PARTICLE PRODUCTION
Descriptors DEC
COSMIC RADIATION; COSMIC SHOWERS; ELEMENTARY PARTICLES; FERMIONS; IONIZING RADIATIONS; LEPTONS; RADIATIONS; SECONDARY COSMIC RADIATION; SHOWERS; SIMULATION