Implications for the Cosmic Ray Spectrum of a Negative Electron Neutrino Mass^2

Simple item page
dc.creatorEhrlich, R.
dc.date1998-12-17
dc.date1999-09-05
dc.date.accessioned2026-07-07T02:29:41Z
dc.date.available2026-07-07T02:29:41Z
dc.descriptionThe features and problems of a speculative model based on the electron neutrino being a tachyon are discussed. The model is consistent with five properties of the cosmic ray spectrum, and it predicts a flux of neutrons in a narrow energy region centered on 4.5 +/- 2.2 x 10^{15} eV.
dc.descriptionPublished in Phys. Rev. D 60, 17302 (1999), 4 pages and 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9812336
dc.identifierhttp://arxiv.org/abs/astro-ph/9812336
dc.identifierPhys.Rev. D60 (1999) 17302
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13571
dc.subjectAstrophysics
dc.titleImplications for the Cosmic Ray Spectrum of a Negative Electron Neutrino Mass^2
dc.typetext

Files

Collections

arXiv