  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 $\Phi_{pp} \propto T^4$ instead of $\Phi_{pp} \propto T^{-1/2}$. 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
