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First 80Se(n,γ) cross section measurement with high resolution in the full stellar energy range 1 eV - 100 keV and its astrophysical implications for the s-process

dc.contributor.authorBabiano-Suarez, V.
dc.contributor.authorBalibrea-Correa, J.
dc.contributor.authorCaballero-Ontanaya, L.
dc.contributor.authorDomingo-Pardo, C.
dc.contributor.authorLadarescu, I.
dc.contributor.authorLerendegui-Marco, J.
dc.contributor.authorTain, J. L.
dc.contributor.authorCalviño, F.
dc.contributor.authorCasanovas, A.
dc.contributor.authorTarifeño-Saldivia, A.
dc.contributor.authorGuerrero, C.
dc.contributor.authorAberle, O.
dc.contributor.authorAlcayne, V.
dc.contributor.authorAmaducci, S.
dc.contributor.authorAndrzejewski, J.
dc.contributor.authorAudouin, L.
dc.contributor.authorBacak, M.
dc.contributor.authorBarbagallo, M.
dc.contributor.authorBennett, S.
dc.contributor.authorBerthoumieux, E.
dc.contributor.authorBillowes, J.
dc.contributor.authorBosnar, D.
dc.contributor.authorBrown, A.
dc.contributor.authorBusso, M.
dc.contributor.authorCaamaño, M.
dc.contributor.authorCalviani, M.
dc.contributor.authorCano-Ott, D.
dc.contributor.authorCerutti, F.
dc.contributor.authorChiaveri, E.
dc.contributor.authorColonna, N.
dc.contributor.authorCortés, G.
dc.contributor.authorCortésGiraldo, M. A.
dc.contributor.authorCosentino, L.
dc.contributor.authorCristallo, S.
dc.contributor.authorDamone, L. A.
dc.contributor.authorDavies, P. J.
dc.contributor.authorDiakaki, M.
dc.contributor.authorDietz, M.
dc.contributor.authorDressler, R.
dc.contributor.authorDucasse, Q.
dc.contributor.authorDupont, E.
dc.contributor.authorDurán, I.
dc.contributor.authorEleme, Z.
dc.contributor.authorFernández-Domínguez, B.
dc.contributor.authorFerrari, A.
dc.contributor.authorFinocchiaro, P.
dc.contributor.authorFurman, V.
dc.contributor.authorGöbel, K.
dc.contributor.authorGarg, R.
dc.contributor.authorGawlik-Ramięga, A.
dc.contributor.authorGilardoni, S.
dc.contributor.authorGonçalves, I. F.
dc.contributor.authorGonzález-Romero, E.
dc.contributor.authorGunsing, F.
dc.contributor.authorHarada, H.
dc.contributor.authorHeinitz, S.
dc.contributor.authorHeyse, J.
dc.contributor.authorJenkins, D. G.
dc.contributor.authorJunghans, A.
dc.contributor.authorKäppeler, F.
dc.contributor.authorKadi, Y.
dc.contributor.authorKimura, A.
dc.contributor.authorKnapová, I.
dc.contributor.authorKokkoris, M.
dc.contributor.authorKopatch, Y.
dc.contributor.authorKrtička, M.
dc.contributor.authorKurtulgil, D.
dc.contributor.authorLederer-Woods, C.
dc.contributor.authorLeeb, H.
dc.contributor.authorLonsdale, S. J.
dc.contributor.authorMacina, D.
dc.contributor.authorManna, A.
dc.contributor.authorMartínez, T.
dc.contributor.authorMasi, A.
dc.contributor.authorMassimi, C.
dc.contributor.authorMastinu, P.
dc.contributor.authorMastromarco, M.
dc.contributor.authorMaugeri, E. A.
dc.contributor.authorMazzone, A.
dc.contributor.authorMendoza, E.
dc.contributor.authorMengoni, A.
dc.contributor.authorMichalopoulou, V.
dc.contributor.authorMilazzo, P. M.
dc.contributor.authorMingrone, F.
dc.contributor.authorMoreno-Soto, J.
dc.contributor.authorMusumarra, A.
dc.contributor.authorNegret, A.
dc.contributor.authorNolte, R.
dc.contributor.authorOgállar, F.
dc.contributor.authorOprea, A.
dc.contributor.authorPatronis, N.
dc.contributor.authorPavlik, A.
dc.contributor.authorPerkowski, J.
dc.contributor.authorPersanti, L.
dc.contributor.authorPetrone, C.
dc.contributor.authorPirovano, E.
dc.contributor.authorPorras, I.
dc.contributor.authorPraena, J.
dc.contributor.authorQuesada, J. M.
dc.contributor.authorRamos-Doval, D.
dc.contributor.authorRauscher, T.
dc.contributor.authorReifarth, R.
dc.contributor.authorRochman, D.
dc.contributor.authorRomanets, Y.
dc.contributor.authorRubbia, C.
dc.contributor.authorSabaté-Gilarte, M.
dc.contributor.authorSaxena, A.
dc.contributor.authorSchillebeeckx, P.
dc.contributor.authorSchumann, D.
dc.contributor.authorSekhar, A.
dc.contributor.authorSmith, A. G.
dc.contributor.authorSosnin, N. V.
dc.contributor.authorSprung, P.
dc.contributor.authorStamatopoulos, A.
dc.contributor.authorTagliente, G.
dc.contributor.authorTassan-Got, L.
dc.contributor.authorThomas, Th.
dc.contributor.authorTorres-Sánchez, P.
dc.contributor.authorTsinganis, A.
dc.contributor.authorUlrich, J.
dc.contributor.authorUrlass, S.
dc.contributor.authorValenta, S.
dc.contributor.authorVannini, G.
dc.contributor.authorVariale, V.
dc.contributor.authorVaz, P.
dc.contributor.authorVentura, A.
dc.contributor.authorVescovi, D.
dc.contributor.authorVlachoudis, V.
dc.contributor.authorVlastou, R.
dc.contributor.authorWallner, A.
dc.contributor.authorWoods, P. J.
dc.contributor.authorWright, T.
dc.contributor.authorŽugec, P.
dc.contributor.authorCollaboration, and the n_TOF
dc.date.accessioned2024-05-21T12:45:03Z
dc.date.available2024-05-21T12:45:03Z
dc.date.issued2022-02-24
dc.identifier.citationBabiano-Suarez , V , Balibrea-Correa , J , Caballero-Ontanaya , L , Domingo-Pardo , C , Ladarescu , I , Lerendegui-Marco , J , Tain , J L , Calviño , F , Casanovas , A , Tarifeño-Saldivia , A , Guerrero , C , Aberle , O , Alcayne , V , Amaducci , S , Andrzejewski , J , Audouin , L , Bacak , M , Barbagallo , M , Bennett , S , Berthoumieux , E , Billowes , J , Bosnar , D , Brown , A , Busso , M , Caamaño , M , Calviani , M , Cano-Ott , D , Cerutti , F , Chiaveri , E , Colonna , N , Cortés , G , CortésGiraldo , M A , Cosentino , L , Cristallo , S , Damone , L A , Davies , P J , Diakaki , M , Dietz , M , Dressler , R , Ducasse , Q , Dupont , E , Durán , I , Eleme , Z , Fernández-Domínguez , B , Ferrari , A , Finocchiaro , P , Furman , V , Göbel , K , Garg , R , Gawlik-Ramięga , A , Gilardoni , S , Gonçalves , I F , González-Romero , E , Gunsing , F , Harada , H , Heinitz , S , Heyse , J , Jenkins , D G , Junghans , A , Käppeler , F , Kadi , Y , Kimura , A , Knapová , I , Kokkoris , M , Kopatch , Y , Krtička , M , Kurtulgil , D , Lederer-Woods , C , Leeb , H , Lonsdale , S J , Macina , D , Manna , A , Martínez , T , Masi , A , Massimi , C , Mastinu , P , Mastromarco , M , Maugeri , E A , Mazzone , A , Mendoza , E , Mengoni , A , Michalopoulou , V , Milazzo , P M , Mingrone , F , Moreno-Soto , J , Musumarra , A , Negret , A , Nolte , R , Ogállar , F , Oprea , A , Patronis , N , Pavlik , A , Perkowski , J , Persanti , L , Petrone , C , Pirovano , E , Porras , I , Praena , J , Quesada , J M , Ramos-Doval , D , Rauscher , T , Reifarth , R , Rochman , D , Romanets , Y , Rubbia , C , Sabaté-Gilarte , M , Saxena , A , Schillebeeckx , P , Schumann , D , Sekhar , A , Smith , A G , Sosnin , N V , Sprung , P , Stamatopoulos , A , Tagliente , G , Tassan-Got , L , Thomas , T , Torres-Sánchez , P , Tsinganis , A , Ulrich , J , Urlass , S , Valenta , S , Vannini , G , Variale , V , Vaz , P , Ventura , A , Vescovi , D , Vlachoudis , V , Vlastou , R , Wallner , A , Woods , P J , Wright , T , Žugec , P & Collaboration , A T NTOF 2022 , ' First 80 Se(n,γ) cross section measurement with high resolution in the full stellar energy range 1 eV - 100 keV and its astrophysical implications for the s-process ' , Paper presented at 16th Symposium on Nuclei in the Cosmos, NIC-XVI 2021 , Chengdu , China , 21/09/21 - 25/09/21 pp. 1-8 . https://doi.org/10.1051/epjconf/202226011026
dc.identifier.citationconference
dc.identifier.otherRIS: urn:23BD7FD6943FD31FAD38CB0F1E7CB002
dc.identifier.otherRIS: 10.1051epjconf202226011026
dc.identifier.urihttp://hdl.handle.net/2299/27903
dc.description© The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).
dc.description.abstractMost elements heavier than iron have been generated in the stellar media by means of neutron capture reactions, approximately half are produced by the slow neutron capture or s-process. Radiative neutron capture cross section measurements are of fundamental importance for the study of this mechanism. In this contribution we present a brief summary on the measurement and results for the 80Se(n,γ) cross-section. The experiment was carried out at CERN n_TOF EAR1 via the time of flight (ToF) technique, using four C6D6 scintillation detectors with very fast response. More than a hundred new resonances have been analyzed for the first time with a high accuracy. The MACS obtained at kT = 8 keV is 36% smaller than the recommended value in KADoNiS. Some of the astrophysical implications of this result are elucidated in this contribution.en
dc.format.extent8
dc.format.extent1848059
dc.language.isoeng
dc.relation.ispartof
dc.subjectNuclear and High Energy Physics
dc.titleFirst 80Se(n,γ) cross section measurement with high resolution in the full stellar energy range 1 eV - 100 keV and its astrophysical implications for the s-processen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85183859959&partnerID=8YFLogxK
rioxxterms.versionofrecord10.1051/epjconf/202226011026
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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