Measurement of near-threshold proton branching ratios in $^{31}$S using $^{28}$Si($^6$Li,t)$^{31}$S(p)$^{30}$P
ORAL
Abstract
The $^{30}$P(p,$\gamma$) reaction is a key step in the nucleosynthesis of elements up to A=40 in models of ONe nova explosions. Prior studies involving particle and/or gamma-ray detection have constrained branching ratios and resonance strengths of a few states in $^{31}$S close to the proton threshold. However, similar information is lacking for a few other states with center-of-mass energy less than 600keV, which is important to determine the reaction rate. In this study, we used the reaction $^{28}$Si($^6$Li,t) to probe a few resonances in this region using the Super-Enge Split-Pole Spectrograph (SE-SPS) at the FSU . Proton decays from $^{31}$S states were detected in coincidence with tritons using the Silicon Array For Branching Ratio Experiments(SABRE). The experimental setup, preliminary results, and astrophysical implications will be discussed.
*This work was supported by FSU NSF Grant No. PHY-2012522, US Department Of Energy grants No. DE-SC0014231 and DE-FG02-96ER40978.
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Presenters
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Balakrishnan Sudarsan
- Louisiana State University
- Louisiana State University, Baton Rouge, LA.