One- and two-neutron capture reactions of light nuclei in nuclear astrophysics
H. Herndl, R. Hofinger, H. Oberhummer
Abstract
We discuss models to calculate one- and two-neutron capture reactions on light nuclei. These are applied to calculate the reaction rates of 15N(n,gamma)16N, 16N(n,gamma)17N and 4He(2n,gamma)6He. The possible astrophysical importance is discussed.
Create a lesson
Related papers
Prospects for modelling odd and odd-odd nuclei using energy density functionals
A. V. Afanasjev, B. Bally, M. Bender et al.
Fast Monte Carlo calculation of multiple scattering in resonant neutron capture
R. M. Djilkibaev
Constraining three-nucleon forces in nuclear lattice effective field theory
Serdar Elhatisari, Ulf-G. Meißner, Zhengxue Ren et al.
Collective-flow signatures of bubble nuclei in intermediate-energy projectile fragmentation reactions
Ge Ren, Chun-Wang Ma, Xi-Guang Cao et al.
R-process nuclei in the rare-earth region above N=126 in Relativistic Hartree-Bogoliubov theory: A preponderance of shape-coexistence in nuclei
M. M. Sharma
Binding energies in the 0-+ and 1-- fermion--antifermion channels from the ladder Bethe-Salpeter and Schrödinger equations
Wei He, Hai-Qing Zhou