Author/Authors :
D. Mocelj، نويسنده , , T. RAUSCHER، نويسنده , , K. Langanke، نويسنده , , G. Martinez-Pinedo، نويسنده , , L. Pacearescu، نويسنده , , Steven A. Fassler، نويسنده , , F.-K. Thielemann، نويسنده ,
Abstract :
Astrophysical reaction rates are sensitive to the parity distribution at low excitation energies. We combine a formula for the energy-dependent parity distribution with a microscopic-macroscopic nuclear level density. This approach describes well the transition from low excitation energies where a single parity dominates to high excitations where the two densities are equal.