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.
Original language | English |
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Pages (from-to) | S1927-S1930 |
Number of pages | 4 |
Journal | Journal of Physics G: Nuclear and Particle Physics |
Volume | 31 |
Issue number | 10 |
DOIs | |
Publication status | Published - Oct 2005 |
Event | 1st International Conference on Nuclear, Structure, Astrophysics and Reactions (NUSTAR 05) - Guildford Duration: 5 Jan 2005 → 8 Jan 2005 |