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dc.contributor.authorOberhummer, H.
dc.contributor.authorKrauss, H.
dc.contributor.authorGrun, K.
dc.contributor.authorRauscher, T.
dc.contributor.authorAbele, H.
dc.contributor.authorMohr, P.
dc.contributor.authorStaudt, G.
dc.date.accessioned2013-07-02T14:32:06Z
dc.date.available2013-07-02T14:32:06Z
dc.date.issued1994-09
dc.identifier.citationOberhummer , H , Krauss , H , Grun , K , Rauscher , T , Abele , H , Mohr , P & Staudt , G 1994 , ' Alpha-clustering and the stellar nucleosynthesis of carbon ' , Zeitschrift fur Physik A-Hadrons and Nuclei , vol. 349 , no. 3-4 , pp. 241-242 .
dc.identifier.issn0939-7922
dc.identifier.otherPURE: 1636849
dc.identifier.otherPURE UUID: 74a5e5f4-6d9e-4bd5-b344-9e5659f52fe4
dc.identifier.otherWOS: A1994PG39600010
dc.identifier.otherScopus: 0001788945
dc.identifier.urihttp://hdl.handle.net/2299/11042
dc.description.abstractThe astrophysical S-factor and reaction rates for the triple-alpha process are calculated in the direct-capture model. It is shown that the stellar carbon production is extremely sensitive to small variations in the N-N interaction.en
dc.format.extent2
dc.language.isoeng
dc.relation.ispartofZeitschrift fur Physik A-Hadrons and Nuclei
dc.rightsOpen
dc.subjectLIGHT-NUCLEI
dc.subjectSCATTERING
dc.titleAlpha-clustering and the stellar nucleosynthesis of carbonen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeSubmitted Version
dcterms.dateAccepted1994-09
rioxxterms.versionSMUR
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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