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dc.contributor.authorDillmann, I.
dc.contributor.authorDomingo-Pardo, C.
dc.contributor.authorHeil, M.
dc.contributor.authorKaeppeler, F.
dc.contributor.authorWalter, S.
dc.contributor.authorDababneh, S.
dc.contributor.authorRauscher, T.
dc.contributor.authorThielemann, Friedrich-Karl
dc.date.accessioned2013-09-26T08:45:11Z
dc.date.available2013-09-26T08:45:11Z
dc.date.issued2010-01
dc.identifier.citationDillmann , I , Domingo-Pardo , C , Heil , M , Kaeppeler , F , Walter , S , Dababneh , S , Rauscher , T & Thielemann , F-K 2010 , ' Stellar (n,gamma) cross sections of p-process isotopes Part I: Pd-102, Te-120, Ba-130,Ba-132, and Dy-156 ' , Physical Review C (nuclear physics) , vol. 81 , no. 1 , 015801 . https://doi.org/10.1103/PhysRevC.81.015801
dc.identifier.issn2469-9985
dc.identifier.urihttp://hdl.handle.net/2299/11652
dc.description.abstractWe have investigated the (n,gamma) cross sections of p-process isotopes with the activation technique. The measurements were carried out at the Karlsruhe Van de Graaff accelerator using the Li-7(p, n) Be-7 source for simulating a Maxwellian neutron distribution of kT = 25 keV. Stellar cross section measurements are reported for the light p-process isotopes Pd-102, Te-120, Ba-130,Ba-132, and Dy-156. In a following paper the cross sections of Yb-168, W-180, Os-184, Pt-190, and Hg-196 will be discussed. The data are extrapolated to p-process energies by including information from evaluated nuclear data libraries. The results are compared to standard Hauser-Feshbach models frequently used in astrophysics.en
dc.format.extent13
dc.format.extent500946
dc.language.isoeng
dc.relation.ispartofPhysical Review C (nuclear physics)
dc.subjectSTARS
dc.subjectATOMIC WEIGHTS
dc.subjectSTATISTICAL-MODEL CALCULATIONS
dc.subjectNUCLEAR-DATA LIBRARY
dc.subjectELEMENTS
dc.subjectASTROPHYSICAL REACTION-RATES
dc.subjectNUCLEOSYNTHESIS
dc.subjectRP-PROCESS
dc.subjectDATA SHEETS
dc.subjectTELLURIUM
dc.titleStellar (n,gamma) cross sections of p-process isotopes Part I: Pd-102, Te-120, Ba-130,Ba-132, and Dy-156en
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1103/PhysRevC.81.015801
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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