Publication Date:
2016-03-08
Description:
Author(s): L. E. Marcucci, G. Mangano, A. Kievsky, and M. Viviani The astrophysical S factor for the radiative capture d ( p , γ ) He 3 in the energy range of interest for big bang nucleosynthesis (BBN) is calculated using an ab initio approach. The nuclear Hamiltonian retains both two- and three-nucleon interactions—the Argonne v 18 and the Urbana IX, respectively. Both … [Phys. Rev. Lett. 116, 102501] Published Tue Mar 08, 2016
Keywords:
Nuclear Physics
Print ISSN:
0031-9007
Electronic ISSN:
1079-7114
Topics:
Physics
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