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Possible explanation for the tail of the cosmic ray spectrum

descriptionPublicationkeyboard_double_arrow_right Article 01 Jun 2000 Argentina English Publisher:Elsevier BVJournal:Physics Letters B, volume 482, pages 343-348 (issn: 0370-2693, Copyright policy )
Authors: Anchordoqui, Luis Alfredo; Dova, María Teresa; McCauley, T. P.; Reucroft, S.; Swain, J. D.;

doi: 10.1016/s0370-2693(00)00534-7

handle: 11336/98577

Possible explanation for the tail of the cosmic ray spectrum

Abstract

Abstract A re-examination of the energy cosmic ray spectrum above 10 20 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.

Country
Argentina
Related Organizations
Keywords

cosmic ray spectrum, https://purl.org/becyt/ford/1.3, Física, COSMIC RAYS, high energy particle interaction, https://purl.org/becyt/ford/1, Ciencias Exactas

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    		 5
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
5
Average
Average
Average
Green
gold