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dc.contributor.authorKiss, G. G.
dc.contributor.authorRauscher, T.
dc.contributor.authorGyurky, Gy.
dc.contributor.authorSimon, A.
dc.contributor.authorFueloep, Zs.
dc.contributor.authorSomorjai, E.
dc.date.accessioned2013-04-30T07:25:01Z
dc.date.available2013-04-30T07:25:01Z
dc.date.issued2008-11-07
dc.identifier.citationKiss , G G , Rauscher , T , Gyurky , G , Simon , A , Fueloep , Z & Somorjai , E 2008 , ' Coulomb Suppression of the Stellar Enhancement Factor ' , Physical Review Letters , vol. 101 , no. 19 , 191101 . https://doi.org/10.1103/PhysRevLett.101.191101
dc.identifier.issn0031-9007
dc.identifier.otherPURE: 1621185
dc.identifier.otherPURE UUID: 1581ff11-87bc-475e-b15f-2477121c5204
dc.identifier.otherWOS: 000260776300014
dc.identifier.otherScopus: 55749112320
dc.identifier.urihttp://hdl.handle.net/2299/10598
dc.description.abstractIt is commonly assumed that reaction measurements for astrophysics should be preferably performed in the direction of a positive Q value to minimize the impact of the stellar enhancement factor, i.e., the difference between the laboratory rate and the actual stellar rate. We show that the stellar effects can be minimized in the charged particle channel, even when the reaction Q value is negative. As a demonstration, the cross section of the astrophysically relevant (85)Rb(p,n)(85)Sr reaction has been measured by activation between 2.16en
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofPhysical Review Letters
dc.rightsOpen
dc.subjectMODEL
dc.subjectPROCESS NUCLEOSYNTHESIS
dc.subjectFINITE NUCLEI
dc.subjectREACTION-RATES
dc.subjectP-PROCESS
dc.subjectHARD-CORE INTERACTION
dc.titleCoulomb Suppression of the Stellar Enhancement Factoren
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2008-11-07
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1103/PhysRevLett.101.191101
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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