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dc.contributor.authorRauscher, T.
dc.contributor.authorThielemann, Friedrich-Karl
dc.date.accessioned2013-07-02T10:32:08Z
dc.date.available2013-07-02T10:32:08Z
dc.date.issued2004-09
dc.identifier.citationRauscher , T & Thielemann , F-K 2004 , ' Predicted cross-sections for photon-induced particle emission ' , Atomic Data and Nuclear Data Tables , vol. 88 , no. 1 , pp. 1-81 . https://doi.org/10.1016/j.adt.2004.07.001
dc.identifier.issn0092-640X
dc.identifier.otherPURE: 1630509
dc.identifier.otherPURE UUID: 9ddb6d20-9226-4163-a1bd-162bbc199305
dc.identifier.otherWOS: 000224625400001
dc.identifier.otherScopus: 4944255239
dc.identifier.urihttp://hdl.handle.net/2299/11004
dc.description.abstractCross-sections for the photon-induced particle-emission reactions (gamma,n), (gamma,p), and (gamma,alpha) are given for all natural isotopes from Ti to Bi. The target nuclei are assumed to be in their ground states, except for Ta-180 which is naturally occurring as the isomer Ta-180m. The cross-sections are calculated in a statistical model (Hauser-Feshbach) approach and covering an energy range from threshold up to 7.35 MeV above the threshold (14.7 MeV above threshold for (gamma,alpha) reactions). The results are intended to aid conception and analysis of experiments which can also be used to test the methods involved in predicting astrophysical reaction rates for nucleo-synthesis. (C) 2004 Elsevier Inc. All rights reserved.en
dc.format.extent81
dc.language.isoeng
dc.relation.ispartofAtomic Data and Nuclear Data Tables
dc.rightsOpen
dc.subjectGAMMA-PROCESS
dc.subjectSTATISTICAL-MODEL CALCULATIONS
dc.subjectBREMSSTRAHLUNG
dc.subjectHEAVY-ELEMENTS
dc.subjectASTROPHYSICAL REACTION-RATES
dc.subjectS-PROCESS
dc.subjectNUCLEOSYNTHESIS
dc.subjectNUCLEAR ASTROPHYSICS
dc.titlePredicted cross-sections for photon-induced particle emissionen
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.versiontypeSubmitted Version
dcterms.dateAccepted2004-09
rioxxterms.versionSMUR
rioxxterms.versionofrecordhttps://doi.org/10.1016/j.adt.2004.07.001
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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