Measurement of <sup>19</sup>Ne Excited States Relevant to the <sup>18</sup>F(p,α)<sup>15</sup>O Reaction in Classical Novae
ORAL
Abstract
Classical novae emit intense γ-ray radiation, primarily at 511-keV due to electron-positron annihilation, with the 18F isotope contributing most to observable emissions due to its relatively long half-life. The abundance of 18F in classical novae is mainly controlled by the primary destruction pathway, 18F(p,α)15O, which proceeds through excited states in the compound nucleus 19Ne. Precise abundance calculations of 18F remain hindered largely due to uncertainties in the proton branching ratios of higher-lying states and the Jπ values of the sub- and near-threshold states in 19Ne. In order to more precisely determine the properties of these states, we conducted a 19F(3He,t)19Ne transfer reaction study using the Super-Enge Split-Pole Spectrograph (SE-SPS) at the Fox Accelerator Laboratory at Florida State University. Proton and alpha decays were collected by the Silicon Array for Branching Ratio Experiments (SABRE) in coincidence with the triton reaction products detected at the focal plane. Results for branching ratios and Jπ values of excited states in 19Ne will be presented.
*This work is supported by FSU NSF grant No. PHY-1712953, and US Department of Energy grant No. DE-SC0014231 and DE-FG02-96ER40978.
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Presenters
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Khang H Pham
- Louisiana State University