Cargando…
Calculation of secondary particles in atmosphere and hadronic interactions
Calculation of secondary particles produced by the interaction of cosmic rays with the nuclei of Earth's atmosphere pose important requirements to particle production models. Here we summarize the important features of hadronic simulations, stressing the importance of the so called ``microscopi...
Autores principales: | Battistoni, G, Ferrari, A, Sala, P R |
---|---|
Lenguaje: | eng |
Publicado: |
2002
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1142/S0217751X02011242 http://cds.cern.ch/record/538985 |
Ejemplares similares
-
The FLUKA atmospheric neutrino flux calculation
por: Battistoni, G., et al.
Publicado: (2002) -
Progresses in the validation of the FLUKA atmospheric $\nu$ flux calculation
por: Battistoni, G., et al.
Publicado: (2001) -
Comparison of the FLUKA calculations with CAPRICE94 data on muons in atmosphere
por: Battistoni, G., et al.
Publicado: (2001) -
High energy extension of the FLUKA atmospheric neutrino flux
por: Battistoni, G., et al.
Publicado: (2003) -
Atmospheric neutrinos in a Large Liquid Argon detector
por: Battistoni, G., et al.
Publicado: (2006)