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dc.contributor.authorWinkler, S.
dc.contributor.authorKrauss, H.
dc.contributor.authorGrun, K.
dc.contributor.authorRauscher, T.
dc.contributor.authorOberhummer, H.
dc.contributor.authorAbele, H.
dc.contributor.authorStaudt, G.
dc.date.accessioned2013-07-31T13:03:02Z
dc.date.available2013-07-31T13:03:02Z
dc.date.issued1992-08
dc.identifier.citationWinkler , S , Krauss , H , Grun , K , Rauscher , T , Oberhummer , H , Abele , H & Staudt , G 1992 , ' Calculation of the He-3(He-3, 2p)He-4 AND H-3(H-3, 2N)He-4 astrophysical S-factor at low energies ' , Journal of Physics G: Nuclear and Particle Physics , vol. 18 , no. 8 , pp. L147-L152 .
dc.identifier.issn0954-3899
dc.identifier.otherPURE: 1637096
dc.identifier.otherPURE UUID: af9e70cc-8446-4d9f-9ae1-fb51a2e85cf6
dc.identifier.otherWOS: A1992JG80100004
dc.identifier.urihttp://hdl.handle.net/2299/11241
dc.description.abstractWe have calculated the cross sections for the charge symmetric reactions He-3(He-3,2p)He-4 and He-3(He-3,2p)He-4 at sub-Coulomb energies in the potential model. Good agreement with the experimental data is obtained. The astrophysical S factors in the thermonuclear energy range are calculated.en
dc.format.extent6
dc.language.isoeng
dc.relation.ispartofJournal of Physics G: Nuclear and Particle Physics
dc.subjectFUSION
dc.subjectSCATTERING
dc.subjectCROSS-SECTIONS
dc.subjectALPHA
dc.titleCalculation of the He-3(He-3, 2p)He-4 AND H-3(H-3, 2N)He-4 astrophysical S-factor at low energiesen
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
dcterms.dateAccepted1992-08
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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