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Experimental simulation of a stellar photon bath by bremsstrahlung: the astrophysical gamma-process

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.date.accessioned2013-06-19T09:00:48Z
dc.date.available2013-06-19T09:00:48Z
dc.date.issued2000-08-31
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.issn0370-2693
dc.identifier.urihttp://hdl.handle.net/2299/10861
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.format.extent4
dc.language.isoeng
dc.relation.ispartofPhysical Letters B
dc.subjectP-PROCESS
dc.titleExperimental simulation of a stellar photon bath by bremsstrahlung: the astrophysical gamma-processen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.description.statusPeer reviewed
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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