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dc.contributor.authorGüray, R. T.
dc.contributor.authorÖzkan, N.
dc.contributor.authorYalçln, C.
dc.contributor.authorRauscher, T.
dc.contributor.authorGyürky, Gy
dc.contributor.authorFarkas, J.
dc.contributor.authorFülöp, Zs
dc.contributor.authorHalász, Z.
dc.contributor.authorSomorjai, E.
dc.date.accessioned2015-06-30T14:06:42Z
dc.date.available2015-06-30T14:06:42Z
dc.date.issued2015-05-29
dc.identifier.citationGüray , R T , Özkan , N , Yalçln , C , Rauscher , T , Gyürky , G , Farkas , J , Fülöp , Z , Halász , Z & Somorjai , E 2015 , ' Measurements of Gd 152 (p,γ) Tb 153 and Gd 152 (p,n) Tb 152 reaction cross sections for the astrophysical γ process ' , Physical Review C (nuclear physics) , vol. 91 , no. 5 , 055809 . https://doi.org/10.1103/PhysRevC.91.055809
dc.identifier.issn2469-9985
dc.identifier.urihttp://hdl.handle.net/2299/16119
dc.description.abstractThe total cross sections for the Gd152(p,γ)Tb153 and Gd152(p,n)152Tb reactions have been measured by the activation method at effective center-of-mass energies 3.47≤Ec.m.eff≤7.94 MeV and 4.96≤Ec.m.eff≤7.94 MeV, respectively. The targets were prepared by evaporation of 30.6% isotopically enriched Gd152 oxide on aluminum backing foils, and bombarded with proton beams provided by a cyclotron accelerator. The cross sections were deduced from the observed γ-ray activity, which was detected off-line by an HPGe detector in a low background environment. The results are presented and compared with predictions of statistical model calculations. This comparison supports a modified optical proton+Gd152 potential suggested earlier.en
dc.format.extent8
dc.format.extent350974
dc.language.isoeng
dc.relation.ispartofPhysical Review C (nuclear physics)
dc.subjectNuclear and High Energy Physics
dc.titleMeasurements of Gd 152 (p,γ) Tb 153 and Gd 152 (p,n) Tb 152 reaction cross sections for the astrophysical γ processen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1103/PhysRevC.91.055809
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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