Abstract
The 30S(α,p)33Cl reaction may have a significant impact on final elemental abundances and energy output of type I X-ray bursts, as well as influencing observables such as double-peaked luminosity profiles, because it could bypass the 30S waiting point. This reaction has been studied experimentally for the first time in inverse kinematics via the time-inverse reaction 1H(33Cl,30S)α with a 33Cl radioactive ion beam produced at the Argonne Tandem Linac Accelerator System facility by the "in-flight" technique. This reaction was studied at three different beam energies. The experimental method used and the resulting data are discussed.
Original language | English |
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Article number | 045802 |
Journal | Physical Review C - Nuclear Physics |
Volume | 84 |
Issue number | 4 |
DOIs | |
State | Published - 6 Oct 2011 |