Abstract
The relevant gamma energy range is explicitly identified where additional gamma strength must be located to have an impact on astrophysically relevant reactions. It is shown that folding the energy dependences of the transmission coefficients and the level density leads to maximal contributions for gamma energies of 2
| Original language | English |
|---|---|
| Article number | 032801 |
| Number of pages | 5 |
| Journal | Physical Review C (nuclear physics) |
| Volume | 78 |
| Issue number | 3 |
| DOIs | |
| Publication status | Published - Sept 2008 |
Keywords
- PHOTON SCATTERING
- R-PROCESS
- PROCESS NUCLEOSYNTHESIS
- DENSITY
- RATES
- MODES
- DIPOLE STRENGTH
- NUCLEI
- NEUTRON
- CROSS-SECTION