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dc.contributor.authorSomorjai, E.
dc.contributor.authorFulop, Zs.
dc.contributor.authorKiss, A.Z.
dc.contributor.authorRolfs, C.E.
dc.contributor.authorTrautvetter, H.P.
dc.contributor.authorGreife, U.
dc.contributor.authorJunker, M.
dc.contributor.authorGoriely, S.
dc.contributor.authorArnould, M.
dc.contributor.authorRayet, M.
dc.contributor.authorRauscher, T.
dc.contributor.authorOberhummer, H.
dc.contributor.editorMezzacappa, A.
dc.date.accessioned2014-11-27T09:59:33Z
dc.date.available2014-11-27T09:59:33Z
dc.date.issued1998
dc.identifier.citationSomorjai , E , Fulop , Z , Kiss , A Z , Rolfs , C E , Trautvetter , H P , Greife , U , Junker , M , Goriely , S , Arnould , M , Rayet , M , Rauscher , T & Oberhummer , H 1998 , Comparison of experimental and calculated S-factors of the p-process reaction Sm-144(alpha,gamma)Gd-148 . in A Mezzacappa (ed.) , Stellar Evolution, Stellar Explosions and Galactic Chemical Evolution . IOP PUBLISHING LTD , Bristol , pp. 607-611 , 2nd Oak Ridge Symposium on Atomic and Nuclear Astrophysics , OAK RIDGE , Tunisia , 2/12/97 .
dc.identifier.citationconference
dc.identifier.isbn0-7503-0555-X
dc.identifier.otherPURE: 1635751
dc.identifier.otherPURE UUID: b1aac4ef-de19-4593-b1b3-25bf54033274
dc.identifier.otherWOS: 000077110500072
dc.identifier.urihttp://hdl.handle.net/2299/14833
dc.description.abstractThe cross section of the Sm-144(alpha,gamma)Gd-148 reaction has been measured at bombarding energies in the 10.5 - 13.4 MeV range using an activation method based on the off-line alpha-activity measurement of the Gd-148 residual nucleus. The long measuring time of the alpha-decay has required the use of etched track detectors. The resulting cross sections and astrophysical S-factors are compared to new statistical model (Hauser-Feshbach) calculations. The experimental data are strongly overestimated by calculations using global alpha - nucleus optical potentials. The calculated values with potential derived from Sm-144+alpha scattering experiment at E-lab=20 MeV are in good agreement with the experimental results at energies E(cm)greater than or equal to 11.5 MeV, however, largely deviate at lower energies. A fitted Woods-Saxon optical potential, describing remarkably well the experimental data in the whole energy region, clearly indicates a strong energy-dependence of the alpha-nucleus potential.en
dc.format.extent5
dc.language.isoeng
dc.publisherIOP PUBLISHING LTD
dc.relation.ispartofStellar Evolution, Stellar Explosions and Galactic Chemical Evolution
dc.titleComparison of experimental and calculated S-factors of the p-process reaction Sm-144(alpha,gamma)Gd-148en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1998
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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