Unmasking the tail of the cosmic ray spectrum

dc.creatorAnchordoqui, Luis Alfredo
dc.creatorDova, María Teresa
dc.creatorMcCauley, Thomas
dc.creatorReucroft, Stephen
dc.creatorSwain, John
dc.date2000-04-27
dc.date2019-09-17T15:03:09Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/81388
dc.identifierhttp://arxiv.org/abs/astro-ph/9912081v2
dc.descriptionA 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 superheavy nuclei (seldom discussed in the literature) is analysed in detail.
dc.descriptionFacultad de Ciencias Exactas
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Exactas
dc.subjectFísica
dc.subjectRadiación cósmica
dc.subjectInteracciones de Partículas Elementales
dc.subjectAltas energías
dc.titleUnmasking the tail of the cosmic ray spectrum
dc.typeArticulo
dc.typePreprint


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