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 |
---|---|
Pages (from-to) | 154-157 |
Number of pages | 4 |
Journal | Nuclear Physics A |
Volume | 758 |
DOIs | |
Publication status | Published - 25 Jul 2005 |
Event | 8th International Symposium on Nucle in the Cosmos (NIC8) - Vancouver, Canada Duration: 19 Jul 2004 → 23 Jul 2004 |