On the balance of the solar p-p chain

Simple item page
dc.creatorCsoto, Attila
dc.date1995-05-24
dc.date.accessioned2026-07-07T05:41:26Z
dc.date.available2026-07-07T05:41:26Z
dc.descriptionI show that the solar neutrino fluxes, predicted by standard nuclear and solar physics, can get closer to the experimental observations if one takes the freedom to introduce two free parameters into the model, as it is done in the MSW solution. I point out that the plasma electron capture of Be7 and the He3(He3,2p)He4 nuclear reactions deserve further experimental and theoretical attention.
dc.descriptionLatex with Revtex
dc.identifierhttps://arxiv.org/abs/nucl-th/9505034
dc.identifierhttp://arxiv.org/abs/nucl-th/9505034
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/82570
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleOn the balance of the solar p-p chain
dc.typetext

Files

Collections

arXiv