Three-body radiative capture reactions

Abstract

Radiative capture reaction rates for ${}^6$He, ${}^9$Be and ${}^{17}$Ne formation at astrophysical conditions are studied within a three-body model using the analytical transformed harmonic oscillator method to calculate their states. An alternative procedure to estimate these rates from experimental data on low-energy breakup is also discussed

arXiv comment4 pages, 3 figures. Proceedings of the VIII Nuclear Physics in Astrophysics international conference (June 2017, Catania, Italy)

References in corpus (11)

• Nuclear Astrophysics
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Cited by in corpus (1)

• Role of resonances in the 8li(p,g)9be capture on reaction rate of the relevant astrophysical synthesis of 9be