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Cosmic Rays from Decaying Vortons

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arxiv astro-ph/9706299 v1 pith:CDRZGHVX submitted 1997-06-30 astro-ph

Luis Masperi , Guillermo Silva This is my paper · ORCID
classification astro-ph
keywords cosmicfluxraysvortonsabundancecarriercoincidentcoming
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abstract

The flux of high energy cosmic rays coming from the decay of vortons is estimated. If the abundance of loops corresponding to a superconductivity scale coincident with that of the string formation is corrected to be compatible with the critical density of universe, it is found that the emission of one carrier per vorton may produce a flux of one cosmic ray event per $km^2$ of detector and per year.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Vortons with Abelian and non-Abelian currents and their stability

    hep-th 2019-09 conditional novelty 5.0 of 10

    Vortons exist numerically in U(1)xU(1) and U(1)xSO(3) global models, obey an approximate Regge relation, decay into spinning Q-balls above a critical frequency, and prefer equatorial internal configurations.

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