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dc.contributor.authorMohr, P.
dc.contributor.authorRauscher, T.
dc.contributor.authorOberhummer, H.
dc.contributor.authorMate, Z.
dc.contributor.authorFulop, Zs.
dc.contributor.authorSomorjai, E.
dc.contributor.authorJaeger, M.
dc.contributor.authorStaudt, G.
dc.date.accessioned2013-07-02T14:02:03Z
dc.date.available2013-07-02T14:02:03Z
dc.date.issued1997-03
dc.identifier.citationMohr , P , Rauscher , T , Oberhummer , H , Mate , Z , Fulop , Z , Somorjai , E , Jaeger , M & Staudt , G 1997 , ' Sm-144-alpha optical potential at astrophysically relevant energies derived from Sm-144(alpha,alpha) Sm-144 elastic scattering ' , Physical Review C , vol. 55 , no. 3 , pp. 1523-1531 .
dc.identifier.issn2469-9985
dc.identifier.otherPURE: 1636048
dc.identifier.otherPURE UUID: 37dd8947-fc44-4dcb-901d-3b09092b0038
dc.identifier.otherWOS: A1997WP32500071
dc.identifier.otherScopus: 0000121510
dc.identifier.urihttp://hdl.handle.net/2299/11037
dc.description.abstractFor the determination of the Sm-144-alpha optical potential we measured the angular distribution bf Sm-144(alpha, alpha)Sm-144 scattering at the energy E(lab)=20 MeV with high accuracy. Using the known systematics pf alpha-nucleus optical potentials we are able to derive the Sm-144-alpha optical potential at the astrophysically relevant energy E(c.m.)=9.5 MeV with very limited uncertainties.en
dc.format.extent9
dc.language.isoeng
dc.relation.ispartofPhysical Review C
dc.subjectCOULOMB BARRIER
dc.subjectTHRESHOLD
dc.subjectALPHA-PARTICLES
dc.subjectHEAVY-ION SCATTERING
dc.titleSm-144-alpha optical potential at astrophysically relevant energies derived from Sm-144(alpha,alpha) Sm-144 elastic scatteringen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionSMUR
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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