Nuclear-reaction kinetics in a quasiequilibrium approximation

Details Nuclear-reaction kinetics in a quasiequilibrium approximation Nuclear-reaction kinetics in a quasiequilibrium approximation

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981sval....7..410k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 7, Dec. 1981, p. 741-747.) Soviet Astronomy Letters, vol. 7, Nov.-Dec. 1981, p. 410-413

Astronomy and Astrophysics

Astrophysics

Approximation, Equilibrium Equations, Nuclear Astrophysics, Nuclear Reactions, Reaction Kinetics, Statistical Distributions, Abundance, Black Holes (Astronomy), Differential Equations, Nuclides, Stellar Evolution

Scientific paper

Nuclear statistical quasi-equilibrium is discussed, with temperature, density, and neutron excess considered as variable factors. The sum of the quasi-equilibrium-group nuclide abundances can also be an independent parameter for the quasi-equilibrium abundance distribution. A differential equation is obtained for the sum, in order to describe the nuclear-reaction kinetics in the quasi-equilibrium approximation.

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