Alpha-clustering and the stellar nucleosynthesis of carbon

dc.contributor.author	Oberhummer, H.
dc.contributor.author	Krauss, H.
dc.contributor.author	Grun, K.
dc.contributor.author	Rauscher, T.
dc.contributor.author	Abele, H.
dc.contributor.author	Mohr, P.
dc.contributor.author	Staudt, G.
dc.date.accessioned	2013-07-02T14:32:06Z
dc.date.available	2013-07-02T14:32:06Z
dc.date.issued	1994-09
dc.identifier.citation	Oberhummer , 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.issn	0939-7922
dc.identifier.other	PURE: 1636849
dc.identifier.other	PURE UUID: 74a5e5f4-6d9e-4bd5-b344-9e5659f52fe4
dc.identifier.other	WOS: A1994PG39600010
dc.identifier.other	Scopus: 0001788945
dc.identifier.uri	http://hdl.handle.net/2299/11042
dc.description.abstract	The 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.extent	2
dc.language.iso	eng
dc.relation.ispartof	Zeitschrift fur Physik A-Hadrons and Nuclei
dc.subject	LIGHT-NUCLEI
dc.subject	SCATTERING
dc.title	Alpha-clustering and the stellar nucleosynthesis of carbon	en
dc.contributor.institution	Centre for Astrophysics Research
dc.description.status	Peer reviewed
rioxxterms.version	SMUR
rioxxterms.type	Journal Article/Review
herts.preservation.rarelyaccessed	true