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dc.date.accessioned 2019-09-19T15:17:19Z
dc.date.available 2019-09-19T15:17:19Z
dc.date.issued 2005-05-30
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/81602
dc.description.abstract The properties of cosmic rays with energies above 106 GeV have to be deduced from the spacetime structure and particle content of the air showers which they initiate. In this review, a summary of the phenomenology of these giant air showers is presented. We describe the hadronic interaction models used to extrapolate results from collider data to ultra high energies, an also the main electromagnetic processes that govern the longitudinal shower evolution as well as the lateral spread of particles. en
dc.language en es
dc.subject Radiación Cósmica es
dc.subject Fenomenología es
dc.subject Cascada atmosférica extensa es
dc.title Phenomenology of cosmic ray air showers en
dc.type Objeto de conferencia es
sedici.identifier.other https://doi.org/10.1142/9789812774439_0005 es
sedici.identifier.isbn 978-981-256-625-6 es
sedici.creator.person Dova, María Teresa 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 Objeto de conferencia 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.date.exposure 2005-01
sedici.relation.event New Worlds in Astroparticle Physics: Fifth International Workshop (Faro, Portugal, 8–10 de enero, 2005) es
sedici.description.peerReview peer-review 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)