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dc.contributor.authorTagliente, G.
dc.contributor.authorMilazzo, P. M.
dc.contributor.authorFujii, K.
dc.contributor.authorAbbondanno, U.
dc.contributor.authorAerts, G.
dc.contributor.authorAlvarez, H.
dc.contributor.authorAlvarez-Velarde, F.
dc.contributor.authorAndriamonje, S.
dc.contributor.authorAndrzejewski, J.
dc.contributor.authorAudouin, L.
dc.contributor.authorBadurek, G.
dc.contributor.authorBaumann, P.
dc.contributor.authorBecvar, F.
dc.contributor.authorBelloni, F.
dc.contributor.authorBerthoumieux, E.
dc.contributor.authorBisterzo, S.
dc.contributor.authorCalvino, F.
dc.contributor.authorCalviani, M.
dc.contributor.authorCano-Ott, D.
dc.contributor.authorCapote, R.
dc.contributor.authorCarrapico, C.
dc.contributor.authorCennini, P.
dc.contributor.authorChepel, V.
dc.contributor.authorChiaveri, E.
dc.contributor.authorColonna, N.
dc.contributor.authorCortes, G.
dc.contributor.authorCouture, A.
dc.contributor.authorCox, J.
dc.contributor.authorDahlfors, M.
dc.contributor.authorDavid, S.
dc.contributor.authorDillmann, I.
dc.contributor.authorDomingo-Pardo, C.
dc.contributor.authorDridi, W.
dc.contributor.authorDuran, I.
dc.contributor.authorEleftheriadis, C.
dc.contributor.authorEmbid-Segura, M.
dc.contributor.authorFerrari, A.
dc.contributor.authorFerreira-Marques, R.
dc.contributor.authorFurman, W.
dc.contributor.authorGallino, R.
dc.contributor.authorGoncalves, I.
dc.contributor.authorGonzalez-Romero, E.
dc.contributor.authorGramegna, F.
dc.contributor.authorGuerrero, C.
dc.contributor.authorGunsing, F.
dc.contributor.authorHaas, B.
dc.contributor.authorHaight, R.
dc.contributor.authorHeil, M.
dc.contributor.authorHerrera-Martinez, A.
dc.contributor.authorRauscher, T.
dc.contributor.authorN TOF Collaboration
dc.date.accessioned2013-11-21T12:20:26Z
dc.date.available2013-11-21T12:20:26Z
dc.date.issued2010-05
dc.identifier.citationTagliente , G , Milazzo , P M , Fujii , K , Abbondanno , U , Aerts , G , Alvarez , H , Alvarez-Velarde , F , Andriamonje , S , Andrzejewski , J , Audouin , L , Badurek , G , Baumann , P , Becvar , F , Belloni , F , Berthoumieux , E , Bisterzo , S , Calvino , F , Calviani , M , Cano-Ott , D , Capote , R , Carrapico , C , Cennini , P , Chepel , V , Chiaveri , E , Colonna , N , Cortes , G , Couture , A , Cox , J , Dahlfors , M , David , S , Dillmann , I , Domingo-Pardo , C , Dridi , W , Duran , I , Eleftheriadis , C , Embid-Segura , M , Ferrari , A , Ferreira-Marques , R , Furman , W , Gallino , R , Goncalves , I , Gonzalez-Romero , E , Gramegna , F , Guerrero , C , Gunsing , F , Haas , B , Haight , R , Heil , M , Herrera-Martinez , A , Rauscher , T & N TOF Collaboration 2010 , ' The Zr-92(n,gamma) reaction and its implications for stellar nucleosynthesis ' , Physical Review C , vol. 81 , no. 5 , 055801 . https://doi.org/10.1103/PhysRevC.81.055801
dc.identifier.issn2469-9985
dc.identifier.otherPURE: 1619062
dc.identifier.otherPURE UUID: d4a7d48a-62b6-4850-b24e-0eda454630f3
dc.identifier.otherWOS: 000278144800074
dc.identifier.otherScopus: 77952469452
dc.identifier.urihttp://hdl.handle.net/2299/12141
dc.description.abstractBecause the relatively small neutron capture cross sections of the zirconium isotopes are difficult to measure, the results of previous measurements are often not adequate for a number of problems in astrophysics and nuclear technology. Therefore, the Zr-92(n,gamma) cross section has been remeasured at the CERN n_TOF facility, providing a set of improved parameters for 44 resonances in the neutron energy range up to 40 keV. With this information the cross-section uncertainties in the keV region could be reduced to 5% as required for s-process nucleosynthesis studies and technological applicationsen
dc.format.extent9
dc.language.isoeng
dc.relation.ispartofPhysical Review C
dc.subjectENERGY RANGE
dc.subjectGIANT BRANCH STARS
dc.subjectCAPTURE CROSS-SECTIONS
dc.subjectFACILITY
dc.subjectN-TOF
dc.subjectELEMENTS
dc.subjectS-PROCESS
dc.subjectZR ISOTOPES
dc.subjectNEUTRON-CAPTURE
dc.subjectCERN
dc.titleThe Zr-92(n,gamma) reaction and its implications for stellar nucleosynthesisen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1103/PhysRevC.81.055801
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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