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dc.contributor.authorGyurky, Gy.
dc.contributor.authorKiss, G. G.
dc.contributor.authorElekes, Z.
dc.contributor.authorFulop, Zs.
dc.contributor.authorSomorjai, E.
dc.contributor.authorPalumbo, A.
dc.contributor.authorGorres, J.
dc.contributor.authorLee, H. Y.
dc.contributor.authorRapp, W.
dc.contributor.authorWiescher, M.
dc.contributor.authorOzkan, N.
dc.contributor.authorGuray, R. T.
dc.contributor.authorEfe, G.
dc.contributor.authorRauscher, T.
dc.date.accessioned2013-04-12T11:44:17Z
dc.date.available2013-04-12T11:44:17Z
dc.date.issued2006-08
dc.identifier.citationGyurky , G , Kiss , G G , Elekes , Z , Fulop , Z , Somorjai , E , Palumbo , A , Gorres , J , Lee , H Y , Rapp , W , Wiescher , M , Ozkan , N , Guray , R T , Efe , G & Rauscher , T 2006 , ' alpha-induced cross sections of Cd-106 for the astrophysical p process ' , Physical Review C (nuclear physics) , vol. 74 , no. 2 , 025805 . https://doi.org/10.1103/PhysRevC.74.025805
dc.identifier.issn2469-9985
dc.identifier.urihttp://hdl.handle.net/2299/10395
dc.description.abstractThe Cd-106(alpha,gamma)Sn-110 reaction cross section has been measured in the energy range of the Gamow window for the astrophysical p-process scenario. The cross sections for Cd-106(alpha,n)Sn-109 and for Cd-106(alpha,p)In-109 below the (alpha,n) threshold have also been determined. The results are compared with predictions of the statistical model code NON-SMOKER using different input parameters. The comparison shows that a discrepancy for Cd-106(alpha,gamma)Sn-110 when using the standard optical potentials can be removed with a different alpha + Cd-106 potential. Some astrophysical implications are discussed.en
dc.format.extent9
dc.format.extent388068
dc.language.isoeng
dc.relation.ispartofPhysical Review C (nuclear physics)
dc.subjectNUCLEAR
dc.subjectSTATISTICAL-MODEL CALCULATIONS
dc.subjectR-PROCESS
dc.subjectENERGIES
dc.subjectMASSIVE STARS
dc.subjectPARTICLES
dc.subjectNEUTRON-STAR MERGERS
dc.subjectNUCLEOSYNTHESIS
dc.subjectGAMMA-PROCESSES
dc.subjectREACTION-RATES
dc.titlealpha-induced cross sections of Cd-106 for the astrophysical p processen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1103/PhysRevC.74.025805
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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