Uncertainties in the18F(p,α)15O reaction rate in classical novae

Abstract

Context.Direct observation ofγ-ray emission from the decay of18F ejected in classical nova outbursts remains a major focus of the nuclear astrophysics community. However, modeling the abundance of ejected18F, and thus the predicted detectability distance of aγ-ray signal near 511 keV emitted from these transient thermonuclear episodes, is hampered by significant uncertainties in our knowledge of the key18F(p,α) reaction rate.Aims.We analyze uncertainties in the most recent nuclear physics experimental results employed to calculate the18F(p,α) reaction rate. Our goal is to determine which uncertainties have the most profound influence on the predicted abundance of18F ejected from novae in order to guide future experimental works.Methods.We calculated a wide range of18F(p,α) reaction rates using theR-Matrix formalism, which allowed us to take all interference effects into account. Using a selection of 16 evenly spaced rates over the full range, we performed 16 new hydrodynamic nova simulations.Results.We have performed one of the most thorough theoretical studies of the impact of the18F(p,α) reaction in classical novae to date. The18F(p,α) rate remains highly uncertain at nova temperatures, resulting in a factor of ∼10 uncertainty in the predicted abundance of18F ejected from nova explosions. We also found that the abundance of18F may be strongly correlated with that of19F.Conclusions.Despite numerous nuclear physics uncertainties affecting the determination of the18F(p,α) reaction rate, dominated by unknown interference signs between 1/2+and 3/2+resonances, future experimental work should focus on firmly and precisely determining the directly measurable quantum properties of the subthreshold states in the compound nucleus19Ne near 6.13 and 6.29 MeV.