Busque entre los 169128 recursos disponibles en el repositorio
Mostrar el registro sencillo del ítem
dc.date.accessioned | 2019-12-05T15:07:19Z | |
dc.date.available | 2019-12-05T15:07:19Z | |
dc.date.issued | 2015 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/86887 | |
dc.description.abstract | We present the first hybrid measurement of the average muon number in air showers at ultrahigh energies, initiated by cosmic rays with zenith angles between 62° and 80°. The measurement is based on 174 hybrid events recorded simultaneously with the surface detector array and the fluorescence detector of the Pierre Auger Observatory. The muon number for each shower is derived by scaling a simulated reference profile of the lateral muon density distribution at the ground until it fits the data. A 1019eV shower with a zenith angle of 67°, which arrives at the surface detector array at an altitude of 1450 m above sea level, contains on average (2.68±0.04±0.48(sys))×107 muons with energies larger than 0.3 GeV. The logarithmic gain dlnNμ/dlnE of muons with increasing energy between 4×1018eV and 5×1019eV is measured to be (1.029±0.024±0.030(sys)). | en |
dc.language | en | es |
dc.subject | Cosmic rays | es |
dc.subject | Hadronic interaction models | es |
dc.title | Muons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events | en |
dc.type | Articulo | es |
sedici.identifier.other | doi:10.1103/PhysRevD.91.032003 | es |
sedici.identifier.other | eid:2-s2.0-84922570220 | es |
sedici.identifier.issn | 1550-7998 | es |
sedici.creator.person | Dova, María Teresa | es |
sedici.creator.person | Hansen, Patricia María | es |
sedici.creator.person | Jarne, Cecilia Gisele | es |
sedici.creator.person | Mariazzi, Analisa Gabriela | es |
sedici.creator.person | Sciutto, Sergio Juan | es |
sedici.creator.person | Wahlberg, Hernán Pablo | es |
sedici.creator.corporate | Pierre Auger Collaboration | es |
sedici.description.note | La lista completa de autores que integran el documento puede consultarse en el archivo | es |
sedici.subject.materias | Física | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Instituto de Física La Plata | es |
sedici.subtype | Articulo | es |
sedici.rights.license | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
sedici.description.peerReview | peer-review | es |
sedici.relation.journalTitle | Physical Review D | es |
sedici.relation.journalVolumeAndIssue | vol. 91, no. 3 | es |
sedici.rights.sherpa | * Color: green * Pre-print del autor: can * Post-print del autor: can * Versión de editor/PDF:can * Condiciones: >>On author's personal website, employer's website or institutional repository >>Institutional repository must not be shared with other institutions >>Publisher's version/PDF may be used >>Link to publisher version required >>Publisher copyright and source must be acknowledged with citation * Link a Sherpa: http://sherpa.ac.uk/romeo/issn/1550-7998/es/ |