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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/


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)