Astrophysically Relevant Neutron Capture near the Border of Stability

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dc.creatorMohr, P.
dc.creatorOberhummer, H.
dc.creatorBeer, H.
dc.date1996-11-21
dc.date.accessioned2026-07-07T05:37:42Z
dc.date.available2026-07-07T05:37:42Z
dc.descriptionThe neutron capture cross section on $^{26}$Mg was measured in the astrophysically relevant energy region from 25 keV to 220 keV. The experimental results agree well with a calculation using the Direct Capture (DC) model together with systematic folding potentials. This experiment confirms for the $^{26}$Mg(n,$γ$)$^{27}$Mg reaction that the DC process is at least comparable to the Compound--Nucleus (CN) process. The reliability of DC calculations is discussed, and we present some ideas for future experiments which could reduce the theoretical uncertainties of DC calculations.
dc.description7 pages (uses sprocl.sty and psfig.sty), 4 figures, Proc. "International Workshop on Research with Fission Fragments", Benediktbeuern, October 28-30, 1996, World Scientific, in press, uuencoded tex-files and postscript-files available at ftp://is1.kph.tuwien.ac.at/pub/ohu/Mg.uu
dc.identifierhttps://arxiv.org/abs/nucl-ex/9611005
dc.identifierhttp://arxiv.org/abs/nucl-ex/9611005
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/81365
dc.subjectNuclear Experiment
dc.subjectNuclear Theory
dc.titleAstrophysically Relevant Neutron Capture near the Border of Stability
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