Dynamics of low-energy nuclear forces and Solar Neutrino Problems in the Nambu-Jona-Lasinio model of light nuclei

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dc.creatorIvanov, A. N.
dc.creatorOberhummer, H.
dc.creatorTroitskaya, N. I.
dc.creatorFaber, M.
dc.date2000-11-04
dc.date.accessioned2026-07-07T01:56:25Z
dc.date.available2026-07-07T01:56:25Z
dc.descriptionThe Solar Neutrino Problems (SNP's) are analysed in the Nambu-Jona-Lasinio model of light nuclei. In this model a possible clue to the solution of the SNP's is in the reduction of the solar neutrino fluxes relative to the predicted by the Standard Solar Model through the decrease of the solar core temperature. The former can be realized through the enhancement of the astrophysical factor for the solar proton burning. The enhancement the upper bound of which is restricted by the helioseismological data goes dynamically via the contribution of the nucleon tensor current coupled to the deuteron. The agreement of the reduced solar neutrino fluxes with the experimental data can be reached within a scenario of vacuum two-flavour neutrino oscillations without a fine tuning of the neutrino-flavour oscillation parameters. In the Nambu-Jona-Lasinio model of light nuclei an enhancement of the astrophysical factor for the solar proton burning entails a change of the cross sections for neutrino and anti-neutrino disintegration of the deuteron at low energies. This provides a theoretical foundation for a new check of a value of the astrophysical factor in terrestrial laboratories.
dc.description18 pages, no figures, Latex
dc.identifierhttps://arxiv.org/abs/astro-ph/0011103
dc.identifierhttp://arxiv.org/abs/astro-ph/0011103
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1993
dc.subjectAstrophysics
dc.titleDynamics of low-energy nuclear forces and Solar Neutrino Problems in the Nambu-Jona-Lasinio model of light nuclei
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