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dc.contributor.authorNassar, H.en
dc.contributor.authorPaul, M.en
dc.contributor.authorAhmad, I.en
dc.contributor.authorBerkovits, D.en
dc.contributor.authorBettan, M.en
dc.contributor.authorCollon, P.en
dc.contributor.authorDababneh, S.en
dc.contributor.authorGhelberg, S.en
dc.contributor.authorGreene, J. P.en
dc.contributor.authorHeger, A.en
dc.contributor.authorHeil, M.en
dc.contributor.authorHenderson, D. J.en
dc.contributor.authorJiang, C. L.en
dc.contributor.authorKappeler, F.en
dc.contributor.authorKoivisto, H.en
dc.contributor.authorO'Brien, S.en
dc.contributor.authorPardo, R. C.en
dc.contributor.authorPatronis, N.en
dc.contributor.authorPennington, T.en
dc.contributor.authorPlag, R.en
dc.contributor.authorRehm, K. E.en
dc.contributor.authorReifarth, R.en
dc.contributor.authorScott, R.en
dc.contributor.authorSinha, S.en
dc.contributor.authorTang, X.en
dc.contributor.authorVondrasek, R.en
dc.date.accessioned2015-11-24T18:34:57Z-
dc.date.available2015-11-24T18:34:57Z-
dc.identifier.issn0031-9007-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17016-
dc.rightsDefault Licence-
dc.subjectmassive starsen
dc.subjection-sourceen
dc.subjects-processen
dc.subjectcaptureen
dc.subjectnucleosynthesisen
dc.subjectseparationen
dc.titleStellar (n,gamma) cross section of Ni-62en
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.primaryDoi 10.1103/Physrevlett.94.092504-
heal.identifier.secondary<Go to ISI>://000227566000017-
heal.identifier.secondaryhttp://prl.aps.org/abstract/PRL/v94/i9/e092504-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate2005-
heal.abstractThe Ni-62(n,gamma)Ni-63(t(1/2) = 100 +/- 2 yr) reaction plays an important role in the control of the flow path of the slow neutron-capture (s) nucleosynthesis process. We have measured for the first time the total cross section of this reaction for a quasi-Maxwellian (kT = 25 keV) neutron flux. The measurement was performed by fast-neutron activation, combined with accelerator mass spectrometry to detect directly the Ni-63 product nuclei. The experimental value of 28.4 +/- 2.8 mb, fairly consistent with a recent calculation, affects the calculated net yield of Ni-62 itself and the whole distribution of nuclei with 62 < A < 90 produced by the weak s process in massive stars.en
heal.journalNamePhys Rev Letten
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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