The level structure of 30S and 31Cl was studied at the NSCL by using neutron removal reactions with a radioactive 31S and 32Cl beam, respectively. The γ -decay from excited states in 30S and 31Cl was measured in a Ge-detector array. The results discussed for this work may reduce the uncertainties in the determination of the 29P(p,γ )30S and 30S(p,γ )31Cl astrophysical reaction rates under rp-process conditions.
|Journal||Proceedings of Science|
|State||Published - 2006|
|Event||9th International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos, NIC 2006 - Geneva, Switzerland|
Duration: Jun 25 2006 → Jun 30 2006