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dc.contributor.authorGyurky, Gy.
dc.contributor.authorFulop, Zs.
dc.contributor.authorKiss, G.
dc.contributor.authorMate, Z.
dc.contributor.authorSomorjai, E.
dc.contributor.authorGorres, J.
dc.contributor.authorPalumbo, A.
dc.contributor.authorWiescher, M.
dc.contributor.authorGalaviz, D.
dc.contributor.authorKretschmer, A
dc.contributor.authorSonnabend, K.
dc.contributor.authorZilges, A.
dc.contributor.authorRauscher, T.
dc.identifier.citationGyurky , G , Fulop , Z , Kiss , G , Mate , Z , Somorjai , E , Gorres , J , Palumbo , A , Wiescher , M , Galaviz , D , Kretschmer , A , Sonnabend , K , Zilges , A & Rauscher , T 2005 , ' A comprehensive study of the Cd-106(alpha, gamma)Sn-110 reaction at energies relevant to the p-process ' , Nuclear Physics A , vol. 758 , pp. 517C-520C .
dc.identifier.otherPURE: 1628109
dc.identifier.otherPURE UUID: 17384b80-31db-41fa-a4df-db751dc97523
dc.identifier.otherWOS: 000230660500111
dc.identifier.otherScopus: 20944446510
dc.description.abstractIn order to test the reliability of reaction rate calculations in the framework of the Hauser-Feshbach statistical model, the cross sections of Cd-106(alpha,gamma)Sn-110 radiative capture reaction were determined in the energy range close to the Gamow window for the astrophysical p-process scenario. In addition, to reduce the errors in the predictions of the statistical model calculations, the relevant optical potential parameters are to be determined from the angular distribution measurement of the Cd-106(alpha, alpha) Cd-106 elastic scattering reaction at low energies.en
dc.relation.ispartofNuclear Physics A
dc.titleA comprehensive study of the Cd-106(alpha, gamma)Sn-110 reaction at energies relevant to the p-processen
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.typeJournal Article/Review

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