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New Maxwellian averaged neutron capture cross sections for Cl-35,Cl-37

dc.contributor.authorGuber, K. H.
dc.contributor.authorSayer, R.O.
dc.contributor.authorValentine, T.E.
dc.contributor.authorLeal, L.C.
dc.contributor.authorSpencer, R.R.
dc.contributor.authorHarvey, J. A.
dc.contributor.authorKoehler, P. E.
dc.contributor.authorRauscher, T.
dc.date.accessioned2013-05-08T08:05:04Z
dc.date.available2013-05-08T08:05:04Z
dc.date.issued2002-05
dc.identifier.citationGuber , K H , Sayer , R O , Valentine , T E , Leal , L C , Spencer , R R , Harvey , J A , Koehler , P E & Rauscher , T 2002 , ' New Maxwellian averaged neutron capture cross sections for Cl-35,Cl-37 ' , Physical Review C , vol. 65 , no. 5 , 058801 . https://doi.org/10.1103/PhysRevC.65.058801
dc.identifier.issn2469-9985
dc.identifier.otherPURE: 1633209
dc.identifier.otherPURE UUID: 044a99b4-8aac-42ec-9125-2d28db702db2
dc.identifier.otherWOS: 000175772600088
dc.identifier.otherScopus: 0036563212
dc.identifier.urihttp://hdl.handle.net/2299/10650
dc.description.abstractThe Oak Ridge Electron Linear Accelerator (ORELA) was used to measure neutron total and capture cross sections of natural chlorine in the energy range from 100 eV to 600 keV. We performed an R-matrix analysis of our new capture and transmission data up to 500 keV. From these resonance parameters new (n, gamma) astrophysical reaction rates were determined over the entire energy range needed by the latest stellar models of the s process.en
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofPhysical Review C
dc.subjectSCATTERING
dc.subjectTRANSMISSION MEASUREMENTS
dc.subjectCL-35
dc.titleNew Maxwellian averaged neutron capture cross sections for Cl-35,Cl-37en
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1103/PhysRevC.65.058801
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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