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dc.contributor.authorMohr, P.
dc.contributor.authorVogt, K.
dc.contributor.authorBabilon, M.
dc.contributor.authorEnders, J.
dc.contributor.authorHartmann, T.
dc.contributor.authorHutter, C.
dc.contributor.authorRauscher, T.
dc.contributor.authorVolz, S.
dc.contributor.authorZilges, A.
dc.identifier.citationMohr , P , Vogt , K , Babilon , M , Enders , J , Hartmann , T , Hutter , C , Rauscher , T , Volz , S & Zilges , A 2000 , ' Experimental simulation of a stellar photon bath by bremsstrahlung: the astrophysical gamma-process ' , Physical Letters B , vol. 488 , no. 2 , pp. 127-130 .
dc.identifier.otherPURE: 1634465
dc.identifier.otherPURE UUID: bdc35f71-1a9e-4bd3-93d8-086937bdb8d8
dc.identifier.otherWOS: 000089213200005
dc.identifier.otherScopus: 0034739111
dc.description.abstractThe nucleosynthesis of heavy proton-rich nuclei in a stellar photon bath at temperatures of the astrophysical gamma-process was investigated where the photon bath was simulated by the superposition of bremsstrahlung spectra with different endpoint energies. The method was applied to derive (gamma,n) cross sections and reaction rates for several platinum isotopes. (C) 2000 Elsevier Science B.V. All rights reserved.en
dc.relation.ispartofPhysical Letters B
dc.titleExperimental simulation of a stellar photon bath by bremsstrahlung: 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

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