| HAL : in2p3-00126590, version 1 |
| arXiv : astro-ph/0611311 |
| DOI : 10.1103/PhysRevLett.101.171101 |
| Fiche détaillée | Récupérer au format |
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| Physical Review Letters 101 (2008) 171101 |
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| Muon Production in Extended Air Shower Simulations |
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| T. PierogK. Werner1 |
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| (2008) |
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| Whereas air shower simulations are very valuable tools for interpreting cosmic ray data, there is a long standing problem: is seems to be impossible to accommodate at the same time the longitudinal development of air showers and the number of muons measured at ground. Using a new hadronic interaction model (EPOS) in air shower simulations produces considerably more muons, in agreement with results from the HiRes-MIA experiment. We find that this is mainly due to a better description of baryon-antibaryon production in hadronic interactions. This is a new aspect of air shower physics which has never been considered so far. |
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| 1 : | SUBATECH - Laboratoire SUBATECH Nantes |
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| Thème(s) | : | Physique/Astrophysique/Cosmologie et astrophysique extra-galactique Physique/Physique des Hautes Energies - Phénoménologie Physique/Physique Nucléaire Expérimentale Physique/Physique Nucléaire Théorique Planète et Univers/Astrophysique |
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| Lien vers le texte intégral : |
| in2p3-00126590, version 1 | |
| http://hal.in2p3.fr/in2p3-00126590 | |
| oai:hal.in2p3.fr:in2p3-00126590 | |
| Contributeur : Dominique Girod | |
| Soumis le : Jeudi 25 Janvier 2007, 13:40:10 | |
| Dernière modification le : Vendredi 9 Octobre 2009, 08:33:58 | |