dc.creatorRoulet, Esteban
dc.date.accessioned2022-09-06T14:53:36Z
dc.date.accessioned2022-10-15T08:22:52Z
dc.date.available2022-09-06T14:53:36Z
dc.date.available2022-10-15T08:22:52Z
dc.date.created2022-09-06T14:53:36Z
dc.date.issued2021-08
dc.identifierRoulet, Esteban; On the relation between the astrophysical neutrino fluxes and the cosmic ray fluxes; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 8; 8-2021; 1-14
dc.identifier1475-7516
dc.identifierhttp://hdl.handle.net/11336/167583
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4364642
dc.description.abstractSome generalizations of the relation between high-energy astrophysical neutrino and cosmic ray fluxes are obtained, taking into account present results on the cosmic ray spectrum and composition as well as a more realistic modeling of the Galactic and extragalactic cosmic ray components down to PeV energies. It is found that the level of neutrino fluxes measured by IceCube can be consistent with sources that are thin to escaping protons. This could also make it easier for heavier nuclei to be emitted from the sources without suffering excessive disintegration processes.
dc.languageeng
dc.publisherIOP Publishing
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1475-7516/2021/08/009
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/1475-7516/2021/08/009
dc.relationinfo:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2105.12506
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectCOSMIC RAY THEORY
dc.subjectULTRA HIGH ENERGY COSMIC RAYS
dc.subjectULTRA HIGH ENERGY PHOTONS AND NEUTRINOS
dc.titleOn the relation between the astrophysical neutrino fluxes and the cosmic ray fluxes
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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