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dc.contributor.authorRauscher, T.
dc.contributor.authorKiss, G. G.
dc.contributor.authorGyuerky, Gy.
dc.contributor.authorSimon, A.
dc.contributor.authorFueloep, Zs.
dc.contributor.authorSomorjai, E.
dc.date.accessioned2013-09-26T08:45:12Z
dc.date.available2013-09-26T08:45:12Z
dc.date.issued2009-09
dc.identifier.citationRauscher , T , Kiss , G G , Gyuerky , G , Simon , A , Fueloep , Z & Somorjai , E 2009 , ' Suppression of the stellar enhancement factor and the reaction Rb-85(p, n)Sr-85 ' , Physical Review C (nuclear physics) , vol. 80 , no. 3 , 035801 . https://doi.org/10.1103/PhysRevC.80.035801
dc.identifier.issn2469-9985
dc.identifier.urihttp://hdl.handle.net/2299/11653
dc.description.abstractIt is shown that a Coulomb suppression of the stellar enhancement factor occurs in many endothermic reactions at and far from stability. Contrary to common assumptions, reaction measurements for astrophysics with minimal impact of stellar enhancement should be preferably performed for those reactions instead of their reverses, despite of their negative Q value. As a demonstration, the cross section of the astrophysically relevant Rb-85(p, n)Sr-85 reaction has been measured by activation between 2.16en
dc.format.extent12
dc.format.extent366464
dc.language.isoeng
dc.relation.ispartofPhysical Review C (nuclear physics)
dc.subjectSTATISTICAL-MODEL CALCULATIONS
dc.subjectR-PROCESS
dc.subjectPROCESS NUCLEOSYNTHESIS
dc.subjectDENSITY
dc.subjectASTROPHYSICAL REACTION-RATES
dc.subjectPHYSICS
dc.subjectFINITE NUCLEI
dc.subjectP-PROCESS
dc.subjectHARD-CORE INTERACTION
dc.subjectTEMPERATURE
dc.titleSuppression of the stellar enhancement factor and the reaction Rb-85(p, n)Sr-85en
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1103/PhysRevC.80.035801
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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