The enhancement factor of the resonant thermonuclear reaction rates is calculated for the extremely dense stellar plasmas in the liquid phase. In order to calculate the enhancement factor we use the screening potential which is deduced from the numerical experiment of the classical one-component plasma. It is found that the enhancement is tremendous for white dwarf densities if the ^{12}C + ^{12}C fusion cross sections show resonant behavior in the astrophysical energy range. We summarize our numerical results by accurate analytic fitting formulae
Electron degeneracy effects are dominant in ultra-dense plasmas (UDP), such as those found in white ...
It is a current opinion that thermonuclear fusion is the main source of the star activity. It is sho...
We analyze thermonuclear and pycnonuclear reaction rates in multi-component dense stellar plasma. Fi...
We argue that the Maxwellian approximation can essentially underestimate the rates of some nuclear r...
The fusion enhancement factor due to screening in the solar plasma is calculated. We use the finite ...
We study two different physical scenarios of thermonuclear reactions in stellar plasmas proceeding t...
The Gamow peak represents one of the most important concepts in the study of thermonuclear reactions...
Recent improvements and remaining problems in the prediction of thermonuclear rates are reviewed. Th...
We study the plasma correlation effects on nonresonant thermonuclear reactions of carbon and oxygen ...
We analyze thermonuclear and pycnonuclear fusion reactions in dense matter containing atomic nuclei ...
"General kinetic equations for nuclear reaction in dense plasmas are obtaincd. They take into accoun...
Due to screening effects, nuclear reactions in astrophysical plasmas may behave differently than in ...
In stellar matter as cool and dense as the interior of a white dwarf, the Coulomb energies between n...
Plasma screening effects affect the rate at which nuclear reactions occur in hot and dense astrophys...
Low-energy cross section data for 86 charged-particle induced reactions involving light (1 less than...
Electron degeneracy effects are dominant in ultra-dense plasmas (UDP), such as those found in white ...
It is a current opinion that thermonuclear fusion is the main source of the star activity. It is sho...
We analyze thermonuclear and pycnonuclear reaction rates in multi-component dense stellar plasma. Fi...
We argue that the Maxwellian approximation can essentially underestimate the rates of some nuclear r...
The fusion enhancement factor due to screening in the solar plasma is calculated. We use the finite ...
We study two different physical scenarios of thermonuclear reactions in stellar plasmas proceeding t...
The Gamow peak represents one of the most important concepts in the study of thermonuclear reactions...
Recent improvements and remaining problems in the prediction of thermonuclear rates are reviewed. Th...
We study the plasma correlation effects on nonresonant thermonuclear reactions of carbon and oxygen ...
We analyze thermonuclear and pycnonuclear fusion reactions in dense matter containing atomic nuclei ...
"General kinetic equations for nuclear reaction in dense plasmas are obtaincd. They take into accoun...
Due to screening effects, nuclear reactions in astrophysical plasmas may behave differently than in ...
In stellar matter as cool and dense as the interior of a white dwarf, the Coulomb energies between n...
Plasma screening effects affect the rate at which nuclear reactions occur in hot and dense astrophys...
Low-energy cross section data for 86 charged-particle induced reactions involving light (1 less than...
Electron degeneracy effects are dominant in ultra-dense plasmas (UDP), such as those found in white ...
It is a current opinion that thermonuclear fusion is the main source of the star activity. It is sho...
We analyze thermonuclear and pycnonuclear reaction rates in multi-component dense stellar plasma. Fi...