EPJ Web Conf.
Volume 165, 2017Nuclear Physics in Astrophysics VIII (NPA8 2017)
|Number of page(s)||4|
|Published online||30 December 2017|
Three-body radiative capture reactions
1 European Centre for Theoretical Studies in Nuclear Physics and Related Areas (ECT*) and Fondazione Bruno Kessler, Villa Tambosi, Strada delle Tabarelle 286, I- 38123 Villazzano (TN), Italy
2 Departamento de Física Atómica, Molecular y Nuclear, Facultad de Física, Universidad de Sevilla, Apartado 1065, E-41080 Sevilla, Spain
3 Centro Nacional de Aceleradores, Universidad de Sevilla, Junta de Andalucía, CSIC, Tomas Alva Edison 7, E-41092 Sevilla, Spain
* e-mail: email@example.com
Published online: 30 December 2017
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.
© The Authors, published by EDP Sciences, 2017
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (http://creativecommons.org/licenses/by/4.0/).
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