2016
DOI: 10.1103/physrevc.94.065803
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Measurement of radiative proton capture onF18and implications for oxygen-neon novae reexamined

Abstract: Background: The rate of the 18 F(p,γ) 19 Ne reaction affects the final abundance of the radioisotope 18 F ejected from novae. This nucleus is important as its abundance is thought to significantly influence the first stage 511 keV and continuum γ-ray emission in the aftermath of novae. No successful measurement of this reaction existed prior to this work, and the rate used in stellar models had been calculated based on incomplete information from contributing resonances. Purpose:Of the two resonances thought t… Show more

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