Nonlocality of the Nucleon Axial Charge and Solar Neutrino Problem

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dc.creatorKochelev, N. I.
dc.date2002-04-19
dc.date2002-04-30
dc.date.accessioned2026-07-07T03:46:50Z
dc.date.available2026-07-07T03:46:50Z
dc.descriptionIt is shown that the specific space distribution of the nucleon axial charge may lead to the significant reduction of the cross section of the reaction $p+p\to D+e^++ν$ and may provide the mechanism to explain observed deficit of solar neutrinos.
dc.description4 pages, 1 figure, Latex
dc.identifierhttps://arxiv.org/abs/hep-ph/0204235
dc.identifierhttp://arxiv.org/abs/hep-ph/0204235
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/41440
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNonlocality of the Nucleon Axial Charge and Solar Neutrino Problem
dc.typetext

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