Gamow-Teller strength in(n,p) reactions at 198 MeV
- 1 March 1995
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review C
- Vol. 51 (3) , 1144-1153
- https://doi.org/10.1103/physrevc.51.1144
Abstract
Measurements of the (n,p) reaction cross section on have been made at 198 MeV for =0–20° in 4° steps. Multipole analyses have been performed on the resulting spectra and Gamow-Teller (GT) strength distributions have been obtained. These GT distributions have been found to occur as strong peaks at low excitation energy in the final Co nuclei and extend weakly upwards to 30 MeV of excitation. Comparisons of the data with renormalized shell-model calculations show reasonable agreement at low excitation, though the calculations predict very little strength at excitation energies above about 6 MeV.
Keywords
This publication has 28 references indexed in Scilit:
- Stellar electron capture rates and the 54Fe(n, p) experimentNuclear Physics A, 1991
- Nuclear data sheets update for A = 64Nuclear Data Sheets, 1991
- Electron capture and beta-decay in presupernova starsThe Astrophysical Journal, 1990
- The (p, n) reaction as a probe of beta decay strengthNuclear Physics A, 1987
- Ratio of the isovector effective interaction strengths ‖Jστ/Jτ‖2 between 200 and 450 MeV from the 14C(p, n) 14N reactionPhysics Letters B, 1986
- Electron capture in stellar collapseNuclear Physics A, 1984
- Analysis of neutron β-decayNuclear Physics A, 1982
- Stellar weak interaction rates for intermediate-mass nuclei. II - A = 21 to A = 60The Astrophysical Journal, 1982
- Nuclear data sheets for A = 64Nuclear Data Sheets, 1979
- Hydrostatic Oxygen Burning in Stars. II. Oxygen Burning at Balanced PowerThe Astrophysical Journal, 1972