Radiative capture reaction for Ne formation within a full three-body model
arXiv:1611.01295 · doi:10.1103/PhysRevC.94.054622
Abstract
Background: The breakout from the hot Carbon-Nitrogen-Oxigen (CNO) cycles can trigger the rp-process in type I x-ray bursts. In this environment, a competition between and the two-proton capture reaction is expected. Purpose: Determine the three-body radiative capture reaction rate for formation including sequential and direct, resonant and non-resonant contributions on an equal footing. Method: Two different discretization methods have been applied to generate Ne states in a full three-body model: the analytical transformed harmonic oscillator method and the hyperspherical adiabatic expansion method. The binary --O interaction has been adjusted to reproduce the known spectrum of the unbound F nucleus. The dominant contributions to the reaction rate have been calculated from the inverse photodissociation process. Results: Three-body calculations provide a reliable description of Ne states. The agreement with the available experimental data on Ne is discussed. It is shown that the reaction rates computed within the two methods agree in a broad range of temperatures. The present calculations are compared with a previous theoretical estimation of the reaction rate. Conclusions: It is found that the full three-body model provides a reaction rate several orders of magnitude larger than the only previous estimation. The implications for the rp-process in type I x-ray bursts should be investigated.
arXiv comment10 pages, 10 figures. Corrected version
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