Add to ORKGText includes handwritten formulasNuclear reaction rates and pressure are calculated using a Maxwellian distribution function which is depleted at its high energy tail. The results are applied to nuclear reactions occuring within the solar interior, showing that the neutrino counting rate can be significantly reduced
We argue that the Maxwellian approximation can essentially underestimate the rates of some nuclear r...
Low-energy cross section data for 86 charged-particle induced reactions involving light (1 less than...
This article illustrates how very small deviations from the Maxwellian exponential tail, while leavi...
Evolutionary sequences for the sun are presented which confirm that the Cl-37 neutrino counting rate...
The physics of nuclear reactions in stellar plasma is reviewed with special emphasis on the importan...
In this work, a standard solar model is computed with new reaction rates that take into account the ...
We discuss the results of Homestake and Kamioka experiments, showing that - if the results of these ...
We review the purely leptonic neutrino emission processes, contributing to the energy loss rate of t...
Density and temperature conditions in the solar core suggest that the microscopic diffusion of elect...
The physics of nuclear reactions in stellar plasma is reviewed with special emphasis on the impor-ta...
Possible modification in the velocity distribution in the non-resonant reaction rates leads to an ex...
We explore the effects of electromagnetic (EM) fluctuations in plasmas on solar neutrino fluxes expl...
We evaluate the effect of electrostatic screening by ions and electrons on low-Z thermonuclear react...
The closed forms of the non-resonant thermonuclear function in the Maxwell–Boltzmann and Tsallis cas...
"General kinetic equations for nuclear reaction in dense plasmas are obtaincd. They take into accoun...
We argue that the Maxwellian approximation can essentially underestimate the rates of some nuclear r...
Low-energy cross section data for 86 charged-particle induced reactions involving light (1 less than...
This article illustrates how very small deviations from the Maxwellian exponential tail, while leavi...
Evolutionary sequences for the sun are presented which confirm that the Cl-37 neutrino counting rate...
The physics of nuclear reactions in stellar plasma is reviewed with special emphasis on the importan...
In this work, a standard solar model is computed with new reaction rates that take into account the ...
We discuss the results of Homestake and Kamioka experiments, showing that - if the results of these ...
We review the purely leptonic neutrino emission processes, contributing to the energy loss rate of t...
Density and temperature conditions in the solar core suggest that the microscopic diffusion of elect...
The physics of nuclear reactions in stellar plasma is reviewed with special emphasis on the impor-ta...
Possible modification in the velocity distribution in the non-resonant reaction rates leads to an ex...
We explore the effects of electromagnetic (EM) fluctuations in plasmas on solar neutrino fluxes expl...
We evaluate the effect of electrostatic screening by ions and electrons on low-Z thermonuclear react...
The closed forms of the non-resonant thermonuclear function in the Maxwell–Boltzmann and Tsallis cas...
"General kinetic equations for nuclear reaction in dense plasmas are obtaincd. They take into accoun...
We argue that the Maxwellian approximation can essentially underestimate the rates of some nuclear r...
Low-energy cross section data for 86 charged-particle induced reactions involving light (1 less than...
This article illustrates how very small deviations from the Maxwellian exponential tail, while leavi...