Production and propagation of heavy hadrons in air-shower simulators

Very energetic charm and bottom hadrons may be produced in the upper atmosphere when a primary cosmic ray or the leading hadron in an extensive air shower collide with a nucleon. At E≈108 GeV their decay length becomes of order 10 km, implying that they tend to interact in the air instead of decayin...

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Detalles Bibliográficos
Autores principales: García Canal, Carlos Alberto, Illana, J. I., Masip, M., Sciutto, Sergio Juan
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2013
Materias:
Física
Astroparticles
Heavy hadrons
Air shower
Simulations
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/97229
https://ri.conicet.gov.ar/11336/23456
https://arxiv.org/abs/1210.7072
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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