A Dynamic Solar Core Model: the SSM-like solution

I point out that all the arguments available in the literature against an astrophysical solution of the solar neutrino problem(s) do not exclude a yet not recognised class of solar models, in which an explosive energy source is present in the solar core besides the standard proton-proton and CNO cycle. It is shown from first principle physics that stars have a non-equilibrium energy source as well, arising from transient local thermonuclear runaways. I derive a model independent inequality, which shows that the problem of the missing beryllium neutrinos lies in that the SuperKamiokande contains a term arising from neutrinos of a non-pp,CNO source. Recent indications suggest strongly that this term plays a more significant role in the solar neutrino problem than neutrino oscillations. The runaways can produce high-energy electrons and high-energy axions, and may produce muon and tau neutrinos above 10 K, and electron antineutrinos. I show that subtracting the runaway term from the SuperKamiokande results the remaining data are compatible with each other, within the frame of a generalised luminosity constraint and standard neutrinos. Allowing non-pp,CNO reaction chains a new approach arises to interpret the neutrino detector data, opening new horizons to solar neutrino astrophysics. I point out, that the temperature dependence of the individual neutrino fluxes is related to pure nuclear physics, but the usual luminosity constraint is model dependent and actually is a questionable assumption. The explicit temperature dependence leads to Φpp ∝ T 4 for the more general case instead of the usual Φpp ∝ T −1/2 for the SSM luminosity constraint. I assume a Sun analogue to the SSM, in the sense that the actual, average temperature can be described by a single parameter, in terms of the SSM temperature. This is the ”SSM-like solution” of the neutrino-flux equations.