Mazzone, A.A.MazzoneCRISTALLO, SergioSergioCRISTALLOAberle, O.O.AberleAlaerts, G.G.AlaertsAlcayne, V.V.AlcayneAmaducci, S.S.AmaducciAndrzejewski, J.J.AndrzejewskiAudouin, L.L.AudouinBabiano-Suarez, V.V.Babiano-SuarezBacak, M.M.BacakBarbagallo, M.M.BarbagalloRadeck, D.D.RadeckRamos Doval, D.D.Ramos DovalReifarth, R.R.ReifarthRochman, D.D.RochmanRubbia, C.C.RubbiaSabaté-Gilarte, M.M.Sabaté-GilarteSAXENA, AAYUSHAAYUSHSAXENASchillebeeckx, P.P.SchillebeeckxSchumann, D.D.SchumannSmith, A. G.A. G.SmithBécares, V.V.BécaresSosnin, N.N.SosninStamatopoulos, A.A.StamatopoulosTagliente, G.G.TaglienteTain, J. L.J. L.TainTalip, Z.Z.TalipTarifeño-Saldivia, A. E.A. E.Tarifeño-SaldiviaTassan-Got, L.L.Tassan-GotTorres-Sánchez, P.P.Torres-SánchezTsinganis, A.A.TsinganisUlrich, J.J.UlrichBečvář, F.F.BečvářUrlass, S.S.UrlassValenta, S.S.ValentaVannini, G.G.VanniniVariale, V.V.VarialeVaz, P.P.VazVentura, A.A.VenturaVESCOVI, DiegoDiegoVESCOVIVlachoudis, V.V.VlachoudisVlastou, R.R.VlastouWallner, A.A.WallnerBellia, G.G.BelliaWoods, P. J.P. J.WoodsWynants, R.R.WynantsWright, T. J.T. J.WrightŽugec, P.P.ŽugecBerthoumieux, E.E.BerthoumieuxBillowes, J.J.BillowesBosnar, D.D.BosnarBrown, A. S.A. S.BrownBusso, M.M.BussoCaamaño, M.M.CaamañoCaballero, L.L.CaballeroCalviani, M.M.CalvianiCalviño, F.F.CalviñoCano-Ott, D.D.Cano-OttCasanovas, A.A.CasanovasCastelluccio, D. M.D. M.CastelluccioCerutti, F.F.CeruttiChen, Y. H.Y. H.ChenChiaveri, E.E.ChiaveriClai, G.G.ClaiColonna, N.N.ColonnaCortés, G. P.G. P.CortésCortés-Giraldo, M. A.M. A.Cortés-GiraldoCosentino, L.L.CosentinoDamone, L. A.L. A.DamoneDiakaki, M.M.DiakakiDietz, M.M.DietzDomingo-Pardo, C.C.Domingo-PardoDressler, R.R.DresslerDupont, E.E.DupontDurán, I.I.DuránEleme, Z.Z.ElemeFernández-Domíngez, B.B.Fernández-DomíngezFerrari, A.A.FerrariFerro-Gonçalves, I.I.Ferro-GonçalvesFinocchiaro, P.P.FinocchiaroFurman, V.V.FurmanGarg, R.R.GargGawlik, A.A.GawlikGilardoni, S.S.GilardoniGlodariu, T.T.GlodariuGöbel, K.K.GöbelGonzález-Romero, E.E.González-RomeroGuerrero, C.C.GuerreroGunsing, F.F.GunsingHeinitz, S.S.HeinitzHeyse, J.J.HeyseJenkins, D. G.D. G.JenkinsJericha, E.E.JerichaKadi, Y.Y.KadiKäppeler, F.F.KäppelerKimura, A.A.KimuraKivel, N.N.KivelKokkoris, M.M.KokkorisKopatch, Y.Y.KopatchKopecky, S.S.KopeckyKrtička, M.M.KrtičkaKurtulgil, D.D.KurtulgilLadarescu, I.I.LadarescuLederer-Woods, C.C.Lederer-WoodsLerendegui-Marco, J.J.Lerendegui-MarcoLo Meo, S.S.Lo MeoLonsdale, S. -J.S. -J.LonsdaleMacina, D.D.MacinaManna, A.A.MannaMartínez, T.T.MartínezMasi, A.A.MasiMassimi, C.C.MassimiMastinu, P. F.P. F.MastinuMastromarco, M.M.MastromarcoMatteucci, F.F.MatteucciMaugeri, E.E.MaugeriMendoza, E.E.MendozaMengoni, A.A.MengoniMichalopoulou, V.V.MichalopoulouMilazzo, P. M.P. M.MilazzoMingrone, F.F.MingroneMucciola, R.R.MucciolaMusumarra, A.A.MusumarraNegret, A.A.NegretNolte, R.R.NolteOgállar, F.F.OgállarOprea, A.A.OpreaPatronis, N.N.PatronisPavlik, A.A.PavlikPerkowski, J.J.PerkowskiPIERSANTI, LucianoLucianoPIERSANTIPorras, I.I.PorrasPraena, J.J.PraenaQuesada, J. M.J. M.Quesada2021-01-212021-01-2120200370-2693http://hdl.handle.net/20.500.12386/29924The neutron capture cross section of <SUP>154</SUP>Gd was measured from 1 eV to 300 keV in the experimental area located 185 m from the CERN n_TOF neutron spallation source, using a metallic sample of gadolinium, enriched to 67% in <SUP>154</SUP>Gd. The capture measurement, performed with four C<SUB>6</SUB>D<SUB>6</SUB> scintillation detectors, has been complemented by a transmission measurement performed at the GELINA time-of-flight facility (JRC-Geel), thus minimising the uncertainty related to sample composition. An accurate Maxwellian averaged capture cross section (MACS) was deduced over the temperature range of interest for s process nucleosynthesis modelling. We report a value of 880(50) mb for the MACS at kT = 30 keV, significantly lower compared to values available in literature. The new adopted <SUP>154</SUP>Gd(n,γ) cross section reduces the discrepancy between observed and calculated solar s-only isotopic abundances predicted by s-process nucleosynthesis models.STAMPAenMeasurement of the 154Gd(n,γ) cross section and its astrophysical implicationsArticle10.1016/j.physletb.2020.1354052-s2.0-85082862606000548740300022http://arxiv.org/abs/2002.02322v1https://www.sciencedirect.com/science/article/pii/S0370269320302094?via%3Dihub2020PhLB..80435405MFIS/04 - FISICA NUCLEARE E SUBNUCLEARE