High energy physics in the atmosphere: phenomenology of cosmic ray air showers

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 we summarize the phenomenology of these giant air showers. We describe the hadronic interaction models used to extrapo...

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Detalles Bibliográficos
Autores principales: Anchordoqui, Luis Alfredo, Dova, María Teresa, Mariazzi, Analisa Gabriela, McCauley, Thomas, Paul, Thomas, Reucroft, Stephen, Swain, John
Formato: Articulo
Lenguaje:Inglés
Publicado: 2004
Materias:
Ciencias Exactas
rayos cósmicos
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/74013
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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