Cosmic Ray and Neutrino Tests of Special Relativity

dc.creatorColeman, Sidney
dc.creatorGlashow, Sheldon L.
dc.date1997-03-05
dc.date1997-04-30
dc.date.accessioned2026-07-07T10:33:29Z
dc.date.available2026-07-07T10:33:29Z
dc.descriptionSearches for anisotropies due to Earth's motion relative to a preferred frame -- modern versions of the Michelson-Morley experiment -- provide precise verifications of special relativity. We describe other tests, independent of this motion, that are or can become even more sensitive. The existence of high-energy cosmic rays places strong constraints on Lorentz non-invariance. Furthermore, if the maximum attainable speed of a particle depends on its identity, then neutrinos, even if massless, may exhibit flavor oscillations. Velocity differences far smaller than any previously probed can produce characteristic effects at accelerators and solar neutrino experiments.
dc.description7 pages, harvmac, 2nd revision discusses recent indications of anisotropy of photons propagating over cosmological distances and is otherwise clarified. Report-no: HUTP-97/A008
dc.identifierhttps://arxiv.org/abs/hep-ph/9703240
dc.identifierhttp://arxiv.org/abs/hep-ph/9703240
dc.identifierPhys.Lett.B405:249-252,1997
dc.identifierdoi:10.1016/S0370-2693(97)00638-2
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179124
dc.subjectHigh Energy Physics - Phenomenology
dc.titleCosmic Ray and Neutrino Tests of Special Relativity
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