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dc.contributor.authorFulop, Zs.
dc.contributor.authorGyurky, Gy.
dc.contributor.authorMate, Z.
dc.contributor.authorSomorjai, E.
dc.contributor.authorZolnai, L.
dc.contributor.authorGalaviz, D.
dc.contributor.authorBabilon, M.
dc.contributor.authorMohr, P.
dc.contributor.authorZilges, A.
dc.contributor.authorRauscher, T.
dc.contributor.authorOberhummer, H.
dc.contributor.authorStaudt, G.
dc.date.accessioned2013-05-09T07:20:03Z
dc.date.available2013-05-09T07:20:03Z
dc.date.issued2001-12
dc.identifier.citationFulop , Z , Gyurky , G , Mate , Z , Somorjai , E , Zolnai , L , Galaviz , D , Babilon , M , Mohr , P , Zilges , A , Rauscher , T , Oberhummer , H & Staudt , G 2001 , ' Mo-92(alpha,alpha)Mo-92 scattering, the Mo-92-alpha optical potential, and the Ru-96(gamma,alpha)Mo-92 reaction rate at astrophysically relevant energies ' , Physical Review C (nuclear physics) , vol. 64 , no. 6 , 065805 . https://doi.org/10.1103/PhysRevC.64.065805
dc.identifier.issn2469-9985
dc.identifier.urihttp://hdl.handle.net/2299/10657
dc.description.abstractThe elastic scattering cross section of (MO)-M-92(alpha,alpha)Mo-92 has been measured at energies of E-c.m. approximate to 13, 16, and 19 MeV in a wide angular range. The real and imaginary parts of the optical potential for the system Mo-92-alpha have been derived at energies around and below the Coulomb barrier, The result fits into the systematic behavior of alpha -nucleus folding potentials. The astrophysically relevant Ru-96(gamma,alpha)Mo-92 reaction rates at, T-9 = 2.0 and T-9 = 3.0 could be determined to an accuracy of about 16% and are compared to previously published theoretical rates.en
dc.format.extent13
dc.format.extent413232
dc.language.isoeng
dc.relation.ispartofPhysical Review C (nuclear physics)
dc.subjectGAMMA-PROCESS
dc.subjectISOTOPES
dc.subjectRANGE
dc.subjectSUPERNOVAE
dc.subjectNUCLEAR ASTROPHYSICS
dc.subjectCROSS-SECTION
dc.subjectINCIDENT ENERGIES
dc.subjectP-PROCESS
dc.titleMo-92(alpha,alpha)Mo-92 scattering, the Mo-92-alpha optical potential, and the Ru-96(gamma,alpha)Mo-92 reaction rate at astrophysically relevant energiesen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1103/PhysRevC.64.065805
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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