A possible solution to the solar neutrino problem: Relativistic corrections to the Maxwellian velocity distribution

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dc.creatorLiu, Jian-Miin
dc.date2001-09-30
dc.date.accessioned2026-07-07T05:46:19Z
dc.date.available2026-07-07T05:46:19Z
dc.descriptionThe relativistic corrections to the Maxwellian velocity distribution are needed for standard solar models. Relativistic equilibrium velocity distribution, if adopted in standard solar models, will lower solar neutrino fluxes and change solar neutrino energy spectra but keep solar sound speeds. It is possibly a solution to the solar neutrino problem.
dc.description4 pages with no figure
dc.identifierhttps://arxiv.org/abs/physics/0110002
dc.identifierhttp://arxiv.org/abs/physics/0110002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/84295
dc.subjectGeneral Physics
dc.titleA possible solution to the solar neutrino problem: Relativistic corrections to the Maxwellian velocity distribution
dc.typetext

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