Astrophysical neutron capture rates in s- and r-process nucleosynthesis

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dc.creatorBeer, H.
dc.creatorMohr, P.
dc.creatorOberhummer, H.
dc.creatorRauscher, T.
dc.creatorMutti, P.
dc.creatorCorvi, F.
dc.creatorSedyshev, P. V.
dc.creatorPopov, Yu. P.
dc.date1997-06-05
dc.date.accessioned2026-07-07T05:37:43Z
dc.date.available2026-07-07T05:37:43Z
dc.descriptionAstrophysical neutron capture rates of light and heavy nuclei have been measured and calculated. For the measurements the activation technique was applied at the 3.75 MV Karlsruhe Van de Graaff accelerator, and at the Geel electron linear accelerator (GELINA) the time-of-flight (TOF) method was used. The calculations were performed using direct and compound nuclear capture models.
dc.description10 pages, uses LaTeX2e with epsf.sty and camready.sty (included), 10 postscript figures with psfig (included), Proceedings of the International Seminar on Interaction of Neutrons with Nuclei, 14.-17 May 1997, Dubna, Russia
dc.identifierhttps://arxiv.org/abs/nucl-ex/9706002
dc.identifierhttp://arxiv.org/abs/nucl-ex/9706002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/81371
dc.subjectNuclear Experiment
dc.subjectNuclear Theory
dc.titleAstrophysical neutron capture rates in s- and r-process nucleosynthesis
dc.typetext

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