Nuclear halo effects in neutron-capture reactions of astrophysical interest

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dc.creatorOberhummer, H.
dc.creatorHerndl, H.
dc.creatorHofinger, R.
dc.creatorYamamoto, Y.
dc.date1996-05-23
dc.date1996-05-28
dc.date.accessioned2026-07-07T09:08:29Z
dc.date.available2026-07-07T09:08:29Z
dc.descriptionThe 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.
dc.description4 pages, 2 postscript figures, uses psfig.sty, to be published in Proceedings of the Eigth Workshop in Nuclear Astrophysics, 22.-27. March 1996, Ringberg Castle, Bad Wiessee, W. Hillebrandt and H. Müller (ed.), uuencoded postscript and tex-files available at ftp://is1.kph.tuwien.ac.at/pub/ohu/Ringberg.uu
dc.identifierhttps://arxiv.org/abs/nucl-th/9605033
dc.identifierhttp://arxiv.org/abs/nucl-th/9605033
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/150737
dc.subjectNuclear Theory
dc.titleNuclear halo effects in neutron-capture reactions of astrophysical interest
dc.typetext

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