Abstract
Radiative capture reaction rates for 6He, 9Be and 17Ne 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.
Cite
CITATION STYLE
APA
Casal, J., Rodríguez-Gallardo, M., Arias, J. M., & Gómez-Camacho, J. (2017). Three-body radiative capture reactions. In EPJ Web of Conferences (Vol. 165). EDP Sciences. https://doi.org/10.1051/epjconf/201716501010
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