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dc.contributor.authorMohr, P.
dc.contributor.authorRauscher, T.
dc.contributor.authorSonnabend, K.
dc.contributor.authorVogt, K.
dc.contributor.authorZilges, A.
dc.date.accessioned2013-07-02T13:02:01Z
dc.date.available2013-07-02T13:02:01Z
dc.date.issued2003-05-05
dc.identifier.citationMohr , P , Rauscher , T , Sonnabend , K , Vogt , K & Zilges , A 2003 , ' Photoreactions in nuclear astrophysics ' , Nuclear Physics A , vol. 718 , pp. 243C-246C . https://doi.org/10.1016/S0375-9474(03)00721-8
dc.identifier.issn0375-9474
dc.identifier.otherPURE: 1632343
dc.identifier.otherPURE UUID: 72ffdb56-b62c-4957-b737-eae8c2b38981
dc.identifier.otherWOS: 000182314300037
dc.identifier.otherScopus: 0038519964
dc.identifier.urihttp://hdl.handle.net/2299/11023
dc.description.abstractCross sections and reaction rates of (gamma,n) reactions have been measured close above threshold with the photoactivation technique. The experimental data for W-186,Pt-190,Pt-192,Pt-198, Hg-196,Hg-198,Hg-204, Au-197, and Pb-204 show good agreement with theoretical predictions.en
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofNuclear Physics A
dc.subjectPHOTON BATH
dc.subjectGAMMA
dc.subjectP-PROCESS
dc.titlePhotoreactions in nuclear astrophysicsen
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.dateAccepted2003-05-05
rioxxterms.versionofrecordhttps://doi.org/10.1016/S0375-9474(03)00721-8
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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