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dc.contributor.authorMosconi, M.en_US
dc.contributor.authorHeil, M.en_US
dc.contributor.authorKappeler, F.en_US
dc.contributor.authorMengoni, A.en_US
dc.contributor.authorPlag, R.en_US
dc.contributor.authorFujii, K.en_US
dc.contributor.authorGallino, R.en_US
dc.contributor.authorAerts, G.en_US
dc.contributor.authorTerlizzi, R.en_US
dc.contributor.authorAbbondanno, U.en_US
dc.contributor.authorÁlvarez-Pol, H.en_US
dc.contributor.authorNeves, F.en_US
dc.contributor.authorPoch, A.en_US
dc.contributor.authorOberhummer, H.en_US
dc.contributor.authorOshima, M.en_US
dc.contributor.authorParadela, Cristinaen_US
dc.contributor.authorO'Brien, S.en_US
dc.contributor.authorPancin, J.en_US
dc.contributor.authorPapachristodoulou, C.en_US
dc.contributor.authorRosetti, M.en_US
dc.contributor.authorPatronis, N.en_US
dc.contributor.authorSarchiapone, L.en_US
dc.contributor.authorPavlik, A.en_US
dc.contributor.authorPretel, C.en_US
dc.contributor.authorPavlopoulos, P.en_US
dc.contributor.authorPerrot, L.en_US
dc.contributor.authorPlompen, A.en_US
dc.contributor.authorPlukis, A.en_US
dc.contributor.authorRubbia, C.en_US
dc.contributor.authorTavora, L.en_US
dc.contributor.authorQuesada, J.en_US
dc.contributor.authorRauscher, T.en_US
dc.contributor.authorVoss, F.en_US
dc.contributor.authorReifarth, R.en_US
dc.contributor.authorRudolf, G.en_US
dc.contributor.authorRullhusen, P.en_US
dc.contributor.authorSalgado, J.en_US
dc.contributor.authorSavvidis, I.en_US
dc.contributor.authorStephan, C.en_US
dc.contributor.authorVannini, G.en_US
dc.contributor.authorTagliente, G.en_US
dc.contributor.authorTaín, José Luisen_US
dc.contributor.authorÁlvarez-Velarde, F.en_US
dc.contributor.authorTassan-Got, L.en_US
dc.contributor.authorVaz, P.en_US
dc.contributor.authorBaumann, P.en_US
dc.contributor.authorVentura, A.en_US
dc.contributor.authorAndriamonje, S.en_US
dc.contributor.authorVillamarin, D.en_US
dc.contributor.authorVincente, M. C.en_US
dc.contributor.authorVlachoudis, V.en_US
dc.contributor.authorVlastou, R.en_US
dc.contributor.authorWalter, S.en_US
dc.contributor.authorAlbornoz, A. C. deen_US
dc.contributor.authorWendler, H.en_US
dc.contributor.authorWisshak, K.en_US
dc.contributor.authorCox, J.en_US
dc.contributor.authorAndrzejewski, Józefen_US
dc.contributor.authorAssimakopoulos, P.en_US
dc.contributor.authorAudouin, L.en_US
dc.contributor.authorBadurek, G.en_US
dc.contributor.authorBevcar, F.en_US
dc.contributor.authorBerthoumieux, Ericen_US
dc.contributor.authorCennini, P.en_US
dc.contributor.authorBisterzo, S.en_US
dc.contributor.authorCalvino, F.en_US
dc.contributor.authorCano Ott, Danielen_US
dc.contributor.authorCapote, R.en_US
dc.contributor.authorChepel, V.en_US
dc.contributor.authorEmbid-Segura, M.en_US
dc.contributor.authorChiaveri, E.en_US
dc.contributor.authorDahlfors, M.en_US
dc.contributor.authorColonna, N.en_US
dc.contributor.authorCortés Rossell, Guillemen_US
dc.contributor.authorCouture, A.en_US
dc.contributor.authorn_TOF Collaboration-
dc.contributor.authorDavid, S.en_US
dc.contributor.authorGoncalves, I.en_US
dc.contributor.authorDillmann, I.en_US
dc.contributor.authorDolfini, R.en_US
dc.contributor.authorHaas, B.en_US
dc.contributor.authorDomingo Pardo, Césaren_US
dc.contributor.authorDridi, W.en_US
dc.contributor.authorDurán, Ignacioen_US
dc.contributor.authorEleftheriadis, C.en_US
dc.contributor.authorFerrant, L.en_US
dc.contributor.authorFerrari, A.en_US
dc.contributor.authorGonzález-Romero, E.en_US
dc.contributor.authorFerreira-Marques, R.en_US
dc.contributor.authorFitzpatrick, L.en_US
dc.contributor.authorFrais-Koelbl, H.en_US
dc.contributor.authorFurman, W.en_US
dc.contributor.authorGoverdovski, A.en_US
dc.contributor.authorMarrone, S.en_US
dc.contributor.authorGramegna, F.en_US
dc.contributor.authorHaight, R.en_US
dc.contributor.authorGriesmayer, E.en_US
dc.contributor.authorGuerrero, C.en_US
dc.contributor.authorGunsing, F.en_US
dc.contributor.authorHerrera-Martínez, A.en_US
dc.contributor.authorIgashira, M.en_US
dc.contributor.authorLindote, A.en_US
dc.contributor.authorIsaev, S.en_US
dc.contributor.authorJericha, E.en_US
dc.contributor.authorKetlerov, V.en_US
dc.contributor.authorKadi, Y.en_US
dc.contributor.authorKaramanis, D.en_US
dc.contributor.authorKaradimos, D.en_US
dc.contributor.authorKerveno, M.en_US
dc.contributor.authorKoehler, P.en_US
dc.contributor.authorKonovalov, V.en_US
dc.contributor.authorLopes, I.en_US
dc.contributor.authorKossionides, E.en_US
dc.contributor.authorKrticka, M.en_US
dc.contributor.authorLamboudis, C.en_US
dc.contributor.authorLeeb, H.en_US
dc.contributor.authorLozano, M.en_US
dc.contributor.authorPapadopoulos, C.en_US
dc.contributor.authorMastinu, P.en_US
dc.contributor.authorLukic, S.en_US
dc.contributor.authorMarganiec, J.en_US
dc.contributor.authorMarques, L.en_US
dc.contributor.authorMilazzo, P. M.en_US
dc.contributor.authorMoreau, C.en_US
dc.date.accessioned2008-12-10T12:35:57Z-
dc.date.available2008-12-10T12:35:57Z-
dc.date.issued2007-01-07en_US
dc.identifier.citationProgress in Particle and Nuclear Physics Vol 59(1): 165-173 (2007)en_US
dc.identifier.issn0146-6410en_US
dc.identifier.urihttp://hdl.handle.net/10261/9168-
dc.description9 pages, 3 figures.-- ISI Article Identifier: 000248204700016en_US
dc.descriptionPrinted version published Jul 2007.-- Issue title: International Workshop on Nuclear Physics 28th Course - Radioactive Beams, Nuclear Dynamics and Astrophysics, Ettore Majorana Center for Scientific Culture (Erice, Sicily, Italy, Sep 16-24, 2006).-
dc.description.abstractThe β-decay of Re-187 (t(1/2) = 42.3 Gyr) represents a suited cosmo-chronometer for the age of the r-process abundances, since the radiogenic part of the daughter isotope Os-187 is defined by the difference between the solar Os-187 abundance and s-process contribution to Os-187. The latter component can be determined via the s-process systematics based on the stellar neutron capture cross sections of Os-186 and Os-187. The laboratory cross section of Os-187 requires a significant correction for the effect of the low-lying excited state at 9.75 keV, which is strongly populated under stellar conditions. This theoretical correction can be improved by an experimental cross section for inelastic scattering to the 9.75 keV state. High resolution time-of-flight measurements of (n, γ) cross sections of Os-186,187,188 from 1 eV to 1 MeV at CERN n_TOF facility are reported. The inferred stellar cross sections differ from previously recommended values. In addition, the inelastic scattering cross section has been measured at 30 keV neutron energy via time-of-flight at the Karlsruhe 3.7 MV Van de Graaff. The implications of these results for the Re/Os clock are discussed.en_US
dc.description.sponsorshipThis work is supported by National Institutions of the related n_TOF participants and partially by EC under contract FIKW-CT-2000-00107.-
dc.format.extent2373 bytes-
dc.format.mimetypetext/plain-
dc.language.isoengen_US
dc.publisherElsevieren_US
dc.rightsclosedAccessen_US
dc.subjectRe/Os cosmo-chronometeren_US
dc.subjects-processen_US
dc.subjectStellar cross sectionsen_US
dc.subjectNeutron captureen_US
dc.subjectInelastic scatteringen_US
dc.titleNeutron reactions and nuclear cosmo-chronologyen_US
dc.typeartículoen_US
dc.identifier.doi10.1016/j.ppnp.2006.12.014-
dc.description.peerreviewedPeer revieweden_US
dc.relation.publisherversionhttps://doi.org/10.1016/j.ppnp.2006.12.014-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.openairetypeartículo-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
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