On the solar neutrino problem in the relativistic field theory model of the deuteron

Simple item page
dc.creatorOberhummer, H.
dc.creatorIvanov, A. N.
dc.creatorTroitskaya, N. I.
dc.creatorFaber, M.
dc.date1997-05-16
dc.date.accessioned2026-07-07T02:23:23Z
dc.date.available2026-07-07T02:23:23Z
dc.descriptionThe relativistic field theory model of the deuteron suggested by us previously is applied to the calculation of the reaction rate of the low-energy two-proton fusion p + p -> D + e+ + nu. The theoretical prediction of the reaction rate obtained is 2.9 times larger than given by the potential approach. This leads to a strong suppression of the high energy solar neutrino fluxes.
dc.description14 pages, LaTeX, plus 1 figure added as postscript file, submitted to Astrophysical Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/9705119
dc.identifierhttp://arxiv.org/abs/astro-ph/9705119
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11224
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleOn the solar neutrino problem in the relativistic field theory model of the deuteron
dc.typetext

Files

Collections

arXiv