Key Ne states identified affecting -ray emission from F in novae
M.R. Hall · D.W. Barbadian · T. Baugher🇺🇸 · A. Lepailleur🇫🇷 · S.D. Pain🇺🇸 · A. Ratkiewicz · S. Ahn🇺🇸 · J.M. Allen🇺🇸 · J.T. Anderson🇺🇸 · A.D. Ayangeakaa🇺🇸 · J.C. Blackmon🇺🇸 · S. Burcher🇺🇸 and 25 other authors
Detection of nuclear-decay rays provides a sensitive thermometer of nova nucleosynthesis. The most intense -ray flux is thought to be annihilation radiation from the decay of F, which is destroyed prior to decay by the F(,)O reaction. Estimates of F production had been uncertain, however, because key near-threshold levels in the compound nucleus, Ne, had yet to be identified. This Letter reports the first measurement of the F(He,)Ne reaction, in which the placement of two long-sought 3/2 levels is suggested via triton-- coincidences. The precise determination of their resonance energies reduces the upper limit of the rate by a factor of at nova temperatures and reduces the average uncertainty on the nova detection probability by a factor of 2.1.