Abstract
In-beam cross section measurements of the Nb-93(p,gamma)Mo-94 reaction have been carried out at E-p = 1.4-4.9 MeV, by using high efficiency high-purity Ge detectors, partly with BGO shields for Compton background suppression. From the resulting cross sections, which lie in the 0.5-300 mub range, astrophysical S factors as well as reaction rates have been obtained. By means of the statistical compound nucleus theory of Hauser and Feshbach, cross sections and reactions rates have also been calculated. A good agreement between the experimental data and the theoretical predictions has been found.
Original language | English |
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Article number | 055804 |
Number of pages | 9 |
Journal | Physical Review C (nuclear physics) |
Volume | 64 |
Issue number | 5 |
DOIs | |
Publication status | Published - Nov 2001 |
Keywords
- ISOTOPES
- MODEL
- ENERGIES
- RATES
- NUCLEAR-LEVEL DENSITY
- LIGHT
- ASTROPHYSICS