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dc.contributor.authorVogt, K.
dc.contributor.authorMohr, P.
dc.contributor.authorRauscher, T.
dc.contributor.authorSonnabend, K.
dc.contributor.authorZilges, A.
dc.date.accessioned2013-07-02T12:47:10Z
dc.date.available2013-07-02T12:47:10Z
dc.date.issued2003-05-05
dc.identifier.citationVogt , K , Mohr , P , Rauscher , T , Sonnabend , K & Zilges , A 2003 , ' Determination of (gamma,n) reaction rates for the astrophysical gamma process ' , Nuclear Physics A , vol. 718 , pp. 575C-577C . https://doi.org/10.1016/S0375-9474(03)00857-1
dc.identifier.issn0375-9474
dc.identifier.otherPURE: 1632195
dc.identifier.otherPURE UUID: 4ad129a3-b5e2-4c52-b7e3-e4de621ff895
dc.identifier.otherWOS: 000182314300119
dc.identifier.otherScopus: 0037572204
dc.identifier.urihttp://hdl.handle.net/2299/11020
dc.description.abstract(gamma,n) cross sections and reaction rates in the astrophysical gamma-process have been measured for the nucleus Pb-204 using the method of photoactivation. Some peculiarities of the (gamma,n) cross.section of this nucleus are discussed.en
dc.format.extent3
dc.language.isoeng
dc.relation.ispartofNuclear Physics A
dc.subjectTHRESHOLD
dc.subjectP-PROCESS
dc.titleDetermination of (gamma,n) reaction rates for the astrophysical gamma processen
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)00857-1
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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