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...
Guardado en:
Autores principales: | Anchordoqui, Luis Alfredo, Dova, María Teresa, Mariazzi, Analisa Gabriela, McCauley, Thomas, Paul, Thomas, Reucroft, Stephen, Swain, John |
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Formato: | Articulo |
Lenguaje: | Inglés |
Publicado: |
2004
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Materias: | |
Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/74013 |
Aporte de: |
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