| Published Articles | |
| Title | Shell-model studies of the astrophysical mirror rp-reactions $^{34}$S (p,y) $^{35}$ C1 and $^{34g,m}$ C1(py)$^{35}Ar |
| Author(s) | Richter, W A (Stellenbosch U.) ; Brown, B Alex (Michigan State U.) ; Longland, R (North Carolina U.) ; Wrede, C (Michigan State U.) ; Fry, C (Michigan State U.) |
| Publication | Geneva : CERN, 2019 |
| Number of pages | 6 |
| In: | CERN Proc. 1 (2019) pp.57-62 |
| In: | Proceedings of the 15th International Conference on Nuclear Reaction Mechanisms, Varenna, Italy, 11 - 15 Jun 2018, pp.57-62 |
| Abstract | The two mirror rp-reactions $^{34}$S (p,y) $^{35}$ C1 and $^{34g,m}$ C1(py)$^{35}$Ar were studied via a shell-model approach. At energies in the resonance region near the proton- emission threshold many negative-parity states appear. We present results of calculations in a full (0+1)hω model space which addresses this problem. Energies, spectroscopic factors and proton-decay widths are calculated for input into the reaction rates. Comparisons are also made with a recent experimental determination of the reaction rate for the first reaction. The thermonuclear $^{34g,m}$C1(py)$^{35}$Ar reaction rates are unknown because of a lack of experimental data. The rates for transitions from the ground state of $^{34}$C1 as well as from the isomeric first excited state of $^{34}$C1 are explicitly calculated taking into account the relative populations of the two states. |
| Copyright/License | the authors |
Corresponding record in: Inspire
レコード 生成： 2019-03-27, 最終変更： 2019-03-29
