A Dynamic Solar Core Model: the Deviant Temperatures Approach
| dc.creator | Grandpierre, Attila | |
| dc.date | 1998-08-31 | |
| dc.date.accessioned | 2026-07-07T02:27:46Z | |
| dc.date.available | 2026-07-07T02:27:46Z | |
| dc.description | I derive here a model independent inequality which shows that the problem of the missing beryllium neutrinos of the Sun roots in the fact that the SuperKamiokande contains a term arising from a non-pp,CNO source. First principle physics shows that the non-pp,CNO source is of thermonuclear runaway origin. Several indications suggest that the non-pp,CNO term plays a more significant role in the solar neutrino problems than neutrino oscillations. When removing the over-restricted SSM luminosity constraint, the temperature dependence of the neutrino fluxes is related to pure nuclear physics and follows $Φ_{pp} \propto T^4$ instead of $Φ_{pp} \propto T^{-1/2}$. The results of the calculations offer solutions to the solar neutrino problems and problems of neutrino oscillations. The dynamic solar model presents predictions to Borexino and SNO measurements. These predictions can serve to distinguish between the MSW and the non-pp,CNO effect. {\it PACS numbers|: 26.65.+t, 26.30.+k, 96.60.JW, 95.30.Cq | |
| dc.description | subm Phys. Rev. Lett | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9808349 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9808349 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12834 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | A Dynamic Solar Core Model: the Deviant Temperatures Approach | |
| dc.type | text |