Reaction rates for Neutron Capture Reactions to C-, N- and O-isotopes to the neutron rich side of stability

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dc.creatorHerndl, H.
dc.creatorHofinger, R.
dc.creatorJank, J.
dc.creatorOberhummer, H.
dc.creatorGoerres, J.
dc.creatorWiescher, M.
dc.creatorThielemann, F. -K.
dc.creatorBrown, B. A.
dc.date1999-08-31
dc.date.accessioned2026-07-07T10:34:39Z
dc.date.available2026-07-07T10:34:39Z
dc.descriptionThe reaction rates of neutron capture reactions on light nuclei are important for reliably simulating nucleosynthesis in a variety of stellar scenarios. Neutron capture reaction rates on neutron-rich C-, N-, and O-isotopes are calculated in the framework of a hybrid compound and direct capture model. The results are tabulated and compared with the results of previous calculations as well as with experimental results.
dc.description33 pages (uses revtex) and 9 postscript figures, accepted for publication in Phys. Rev. C
dc.identifierhttps://arxiv.org/abs/nucl-th/9908087
dc.identifierhttp://arxiv.org/abs/nucl-th/9908087
dc.identifierPhys.Rev.C60:064614,1999
dc.identifierdoi:10.1103/PhysRevC.60.064614
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179545
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.subjectNuclear Experiment
dc.titleReaction rates for Neutron Capture Reactions to C-, N- and O-isotopes to the neutron rich side of stability
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