Nuclear halo effects in neutron-capture reactions of astrophysical interest
H. Oberhummer, H. Herndl, R. Hofinger, Y. Yamamoto
Abstract
The halo effect in the final states of astrophysically relevant direct neutron--capture reactions by neutron--rich nuclei is discussed. As an example, we calculate the cross sections for 18O(n,γ)19O at thermonuclear and thermal energies.
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