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Properties of states in \textsuperscript{19}Ne important for the \textsuperscript{18}F\textsuperscript{15}O reaction rate
K. H. Pham, D. Mumma, C. M. Deibel +22
Observation of the 511-keV positron-annihilation line would be a powerful probe of classical novae, with the primary source of positrons likely from the decay of \textsupersc…
B states above the -decay threshold studied via BB
A. N. Kuchera, G. Ryan, G. Selby +12
The resonance region of B covering excitation energies from 8.4 MeV to 13.6 MeV was investigated with the reaction performed on an enriched B target at the Fl…
Properties of states near = 6 MeV in Ne through F+p scattering
Sudarsan Balakrishnan, Laura E. Linhardt, Jeffery C. Blackmon +11
Background: The rate of energy production in the hot-CNO cycle and breakout to the rapid-proton capture process in Type I X-ray bursts is strongly related to the O()$^{…
Study of the Ar()K reaction rate via proton scattering on K, and its impact on properties of modeled X-Ray bursts
A. Lauer-Coles, C. M. Deibel, J. C. Blackmon +21
Background: Type I X-Ray bursts (XRBs) are energetic stellar explosions that occur on the surface of a neutron star in an accreting binary system with a low-mass H/He-rich companio…
Measurement of the reaction and impact on the reaction rate
Eli Temanson, Jessica Baker, Sean Kuvin +6
The reaction is part of a reaction network with impact on the observed galactic Al abundance. A new determination of the proton strength of th…
Enhancement of fusion at near and sub-barrier energies for neutron-rich light nuclei
Varinderjit Singh, J. Vadas, T. K. Steinbach +8
Measurement of the fusion cross-section for neutron-rich light nuclei is crucial in ascertaining if fusion of these nuclei occurs in the outer crust of a neutron star. We have ther…