Resolution of the Solar Neutrino Anomaly

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dc.creatorDubin, Maurice
dc.creatorSoberman, Robert K.
dc.date1996-04-14
dc.date.accessioned2026-07-07T02:21:08Z
dc.date.available2026-07-07T02:21:08Z
dc.descriptionThe solar neutrino anomaly, measurements discrepant from predictions of the Standard Solar Model, has existed for over 30 years. Multiple experiments measuring fluxes from several reactions in the hydrogen fusion chain have added to the puzzle. Each of the several elements of the enigma are resolved by recognition of measurements establishing that most of the sun's fusion must occur near the surface rather than the core.
dc.description8 pages, 2 Postscript figures, uses revtex.sty
dc.identifierhttps://arxiv.org/abs/astro-ph/9604074
dc.identifierhttp://arxiv.org/abs/astro-ph/9604074
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10440
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleResolution of the Solar Neutrino Anomaly
dc.typetext

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