EPJ Web Conf.
Volume 113, 201621st International Conference on Few-Body Problems in Physics
|Number of page(s)||4|
|Section||Nuclear Structure and Reactions|
|Published online||25 March 2016|
Towards an ab initio description of light-nuclei radiative captures
1 TRIUMF, 4004 Wesbrook Mall, Vancouver BC V6T 2A3, Canada
2 Lawrence Livermore National Laboratory, P.O. Box 808, L-414, Livermore, California 94551, USA
3 Department of Physics, Hokkaido University, Sapporo 060-0810, Japan
a e-mail: firstname.lastname@example.org
Published online: 25 March 2016
The 3He(α, γ)7Be and 3H(α, γ)7Li astrophysical S factors are evaluated at low collision energies (less than 2.5 MeV in the centre-of-mass frame) within the no-core shell model with continuum using a renormalized chiral nucleon-nucleon interaction.
© Owned by the authors, published by EDP Sciences, 2016
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.
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