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dc.contributor.authorBao, Z.Y.
dc.contributor.authorBeer, H.
dc.contributor.authorKappeler, F.
dc.contributor.authorVoss, F.
dc.contributor.authorWisshak, K.
dc.contributor.authorRauscher, T.
dc.date.accessioned2013-06-19T08:45:45Z
dc.date.available2013-06-19T08:45:45Z
dc.date.issued2000-09
dc.identifier.citationBao , Z Y , Beer , H , Kappeler , F , Voss , F , Wisshak , K & Rauscher , T 2000 , ' Neutron cross sections for nucleosynthesis studies ' , Atomic Data and Nuclear Data Tables , vol. 76 , no. 1 , pp. 70-154 . https://doi.org/10.1006/adnd.2000.0838
dc.identifier.issn0092-640X
dc.identifier.otherPURE: 1634409
dc.identifier.otherPURE UUID: 71fb1519-8b38-4580-9057-7e2fdb4641c3
dc.identifier.otherWOS: 000089581600004
dc.identifier.otherScopus: 0004134107
dc.identifier.urihttp://hdl.handle.net/2299/10856
dc.description.abstractPrevious compilations of (n, gamma) cross sections of relevance for neutron capture nucleosynthesis in the big bang and in the slow neutron capture process (s process) have been updated to encompass information available up to December 1998; data references include work in process then and published subsequently. The experimental results for nuclei between H and Bi were critically surveyed, renormalized to selected standard cross sections, and condensed into a set of recommended Maxwellian averaged cross sections for a thermal energy of kT = 30 keV. Recent statistical model calculations of the capture cross sections made with the code NON-SMOKER are listed for comparison; these calculated cross sections are adopted in those cases where experimental information is still missing, e.g., for the majority of radioactive nuclei defining the s-process branchings. Maxwellian averages, normalized to our recommended 30 keV averages, were determined for a range of thermal energies between kT = 5 and 100 keV. We have also included the calculated stellar enhancement factors due to thermally populated nuclear states as a function of temperature. (C) 2000 Academic Press.en
dc.format.extent85
dc.language.isoeng
dc.relation.ispartofAtomic Data and Nuclear Data Tables
dc.subjectTHERMONUCLEAR ENERGIES
dc.subjectNUCLEAR-STRUCTURE
dc.subjectRADIATIVE-CAPTURE
dc.subjectLEVEL DENSITIES
dc.subjectTRANSMISSION MEASUREMENTS
dc.subjectCAPTURE MEASUREMENTS
dc.subjectXENON ISOTOPES
dc.subjectMODEL-CALCULATIONS
dc.subjectS-PROCESS NUCLEOSYNTHESIS
dc.subjectSTELLAR NUCLEOSYNTHESIS
dc.titleNeutron cross sections for nucleosynthesis studiesen
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
dcterms.dateAccepted2000-09
rioxxterms.versionofrecordhttps://doi.org/10.1006/adnd.2000.0838
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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