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Nuclear halo effects in neutron-capture reactions of astrophysical interest

H. Oberhummer·H. Herndl·R. Hofinger·Y. Yamamoto
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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 $^{18}$O(n,$γ$)$^{19}$O at thermonuclear and thermal energies.

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H. Oberhummer, H. Herndl, R. Hofinger, Y. Yamamoto. 1996-05-28. Nuclear halo effects in neutron-capture reactions of astrophysical interest. https://arxiv.org/abs/nucl-th/9605033

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