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dc.contributor.authorSkakun, Ye
dc.contributor.authorRauscher, T.
dc.contributor.editorTanihara, I.
dc.date.accessioned2014-07-31T13:00:29Z
dc.date.available2014-07-31T13:00:29Z
dc.date.issued2010
dc.identifier.citationSkakun , Y & Rauscher , T 2010 , Astrophysical S-Factors and Reaction Rates of Threshold (p,n)-Reactions on (99-102)Ru . in I Tanihara (ed.) , 10th Int Symposium on Origin of Matter and Evolution of Galaxies : OMEG-2010 . AIP Conf Procs , vol. 1269 , American Institute of Physics , pp. 390-393 , 10th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG10) , Osaka , Japan , 8/03/10 . https://doi.org/10.1063/1.3485176
dc.identifier.citationconference
dc.identifier.isbn978-0-7354-0819-7
dc.identifier.issn0094-243X
dc.identifier.otherPURE: 1620026
dc.identifier.otherPURE UUID: 1159283e-dafb-450b-a3a2-a8157709ae4e
dc.identifier.otherWOS: 000281986900067
dc.identifier.otherScopus: 77956626509
dc.identifier.urihttp://hdl.handle.net/2299/14222
dc.description.abstractAstrophysical S-factors of (p,n) reactions on (99)Ru, (100)Ru, (101)Ru, and (102)Ru were derived from the sum of experimental isomeric and ground states cross sections measured in the incident proton energy range of 5-9 MeV. They were compared with Hauser-Feshbach statistical model predictions of the NON-SMOKER code. Good agreement was found in the majority of cases. Reaction rates were derived up to 8.7 GK stellar temperature by combining experiment and theory.en
dc.format.extent4
dc.language.isoeng
dc.publisherAmerican Institute of Physics
dc.relation.ispartof10th Int Symposium on Origin of Matter and Evolution of Galaxies
dc.relation.ispartofseriesAIP Conf Procs
dc.subjectp-process
dc.subjectMODEL
dc.subjectPROCESS NUCLEOSYNTHESIS
dc.subjectCAPTURE CROSS-SECTIONS
dc.subjectstatistical model
dc.subjectRELEVANT
dc.subject(p,n) reactions
dc.subjectreaction rates
dc.subjectGAMMA-PROCESSES
dc.subjectNUCLEAR ASTROPHYSICS
dc.subjectnucleosynthesis
dc.subjectP-PROCESS
dc.titleAstrophysical S-Factors and Reaction Rates of Threshold (p,n)-Reactions on (99-102)Ruen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
rioxxterms.versionofrecordhttps://doi.org/10.1063/1.3485176
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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