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dc.date.accessioned | 2019-09-17T15:10:30Z | |
dc.date.available | 2019-09-17T15:10:30Z | |
dc.date.issued | 1999-05-05 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/81391 | |
dc.description.abstract | An analysis of the differences introduced by the hadronic interaction event generators during the development of the showers is presented. We have generated proton and nuclei induced air showers with energies up to 1020.5 eV, “herded up” by the code AIRES + SIBYLL/QGSJET. The most relevant observables are taken into account for the comparison. | en |
dc.language | en | es |
dc.subject | Cascada atmosférica extensa | es |
dc.subject | AIRES | es |
dc.subject | SIBYLL | es |
dc.subject | QGSJET | es |
dc.title | Extensive air showers rounded up by AIRES + SIBYLL/QGS | en |
dc.type | Articulo | es |
sedici.identifier.uri | http://arxiv.org/abs/hep-ph/9905248v1 | es |
sedici.creator.person | Anchordoqui, Luis Alfredo | es |
sedici.creator.person | Dova, María Teresa | es |
sedici.creator.person | Sciutto, Sergio Juan | es |
sedici.subject.materias | Ciencias Exactas | es |
sedici.subject.materias | Física | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Facultad de Ciencias Exactas | es |
sedici.subtype | Preprint | 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/ |