Possible explanation for the tail of the cosmic ray spectrum

A re-examination of the energy cosmic ray spectrum above 10<SUP>20</SUP> eV is presented. The overall data-base provides evidence, albeit still statistically limited, that non-nucleon primaries could be present at the end of the spectrum. In particular, the possible appearance of superhe...

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Detalles Bibliográficos
Autores principales:	Anchordoqui, Luis Alfredo, Dova, María Teresa, McCauley, T. P., Reucroft, S., Swain, J. D.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2000
Materias:	Ciencias Exactas Física cosmic ray spectrum high energy particle interaction
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/75558
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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