Three-body radiative capture reactions
J. Casal, M. Rodr\'iguez-Gallardo, J. M. Arias, J. G\'omez-Camacho
TL;DR
This paper investigates radiative capture reaction rates for specific light nuclei relevant to astrophysics using a three-body model and introduces an alternative method to estimate these rates from experimental breakup data.
Contribution
It presents a novel application of the analytical transformed harmonic oscillator method for calculating reaction rates and proposes an alternative estimation procedure from experimental data.
Findings
Calculated reaction rates for $^6$He, $^9$Be, and $^{17}$Ne at astrophysical energies.
Validated the three-body model against experimental breakup data.
Provided a new method for estimating reaction rates from experimental observations.
Abstract
Radiative capture reaction rates for He, Be and 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
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