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Recent results in nuclear astrophysics at the n-TOF facility at CERN

dc.contributor.authorTagliente, G.
dc.contributor.authorAberle, O.
dc.contributor.authorAndrzejewski, J.
dc.contributor.authorAudouin, L.
dc.contributor.authorBacak, M.
dc.contributor.authorBalibrea, J.
dc.contributor.authorBarbagallo, M.
dc.contributor.authorBečváf, F.
dc.contributor.authorBerthoumieux, E.
dc.contributor.authorBillowes, J.
dc.contributor.authorBosnar, D.
dc.contributor.authorBrown, A.
dc.contributor.authorCaamaño, M.
dc.contributor.authorCalviño, F.
dc.contributor.authorCalviani, M.
dc.contributor.authorCano-Ott, D.
dc.contributor.authorCardella, R.
dc.contributor.authorCasanovas, A.
dc.contributor.authorCerutti, F.
dc.contributor.authorChen, Y. H.
dc.contributor.authorChiaveri, E.
dc.contributor.authorColonna, N.
dc.contributor.authorCortés, G.
dc.contributor.authorCortés-Giraldo, M. A.
dc.contributor.authorCosentino, C.
dc.contributor.authorDamone, L. A.
dc.contributor.authorDiakaki, M.
dc.contributor.authorDomingo-Pardo, C.
dc.contributor.authorDressler, L. R.
dc.contributor.authorDupont, E.
dc.contributor.authorDurán, I.
dc.contributor.authorFernández-Domínguez, B.
dc.contributor.authorFerrari, A.
dc.contributor.authorFerreira, P.
dc.contributor.authorFinocchiaro, P.
dc.contributor.authorFurman, V.
dc.contributor.authorGöbel, K.
dc.contributor.authorGarcía, A. R.
dc.contributor.authorGawlik, A.
dc.contributor.authorGilardoni, S.
dc.contributor.authorGlodariu, T.
dc.contributor.authorGonçalves, I. F.
dc.contributor.authorGonzález, E.
dc.contributor.authorGriesmayer, E.
dc.contributor.authorGuerrero, C.
dc.contributor.authorGunsing, F.
dc.contributor.authorHarada, H.
dc.contributor.authorHeinitz, S.
dc.contributor.authorHeyse, J.
dc.contributor.authorJenkins, D. G.
dc.contributor.authorJericha, E.
dc.contributor.authorKäppeler, F.
dc.contributor.authorKadi, Y.
dc.contributor.authorKalamara, A.
dc.contributor.authorKavrigin, P.
dc.contributor.authorKimura, A.
dc.contributor.authorKivel, N.
dc.contributor.authorKokkoris, M.
dc.contributor.authorKrtička, M.
dc.contributor.authorKurtulgil, D.
dc.contributor.authorLeal-Cidoncha, E.
dc.contributor.authorLederer, C.
dc.contributor.authorLerendegui-Marco, J.
dc.contributor.authorLeeb, H.
dc.contributor.authorLo Meo, S.
dc.contributor.authorLonsdale, S. J.
dc.contributor.authorMacina, D.
dc.contributor.authorMarganiec, J.
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.authorMingrone, F.
dc.contributor.authorMilazzo, P. M.
dc.contributor.authorMusumarra, A.
dc.contributor.authorNegret, A.
dc.contributor.authorNolte, R.
dc.contributor.authorOprea, A.
dc.contributor.authorPatronis, N.
dc.contributor.authorPavlik, A.
dc.contributor.authorPerkowski, J.
dc.contributor.authorPorras, I.
dc.contributor.authorPraena, J.
dc.contributor.authorQuesada, J. M.
dc.contributor.authorRadeck, D.
dc.contributor.authorRauscher, T.
dc.contributor.authorReifarth, R.
dc.contributor.authorRubbia, C.
dc.contributor.authorRyan, J. A.
dc.contributor.authorSabaté-Gilarte, M.
dc.contributor.authorSaxena, A.
dc.contributor.authorSchillebeeckx, P.
dc.contributor.authorSchumann, D.
dc.contributor.authorSedyshev, P.
dc.contributor.authorSmith, A. G.
dc.contributor.authorSosnin, N. V.
dc.contributor.authorStamatopoulos, A.
dc.contributor.authorTain, J. L.
dc.contributor.authorTarifeño-Saldivia, A.
dc.contributor.authorTassan-Got, L.
dc.contributor.authorValenta, S.
dc.contributor.authorVannini, G.
dc.contributor.authorVariale, V.
dc.contributor.authorVaz, P.
dc.contributor.authorVentura, A.
dc.contributor.authorVlachoudis, V.
dc.contributor.authorVlastou, R.
dc.contributor.authorWallner, A.
dc.contributor.authorWarren, S.
dc.contributor.authorWoods, P. J.
dc.contributor.authorWright, T.
dc.contributor.authorZugec, P.
dc.date.accessioned2019-10-17T00:02:35Z
dc.date.available2019-10-17T00:02:35Z
dc.date.issued2016-09-11
dc.identifier.citationTagliente , G , Aberle , O , Andrzejewski , J , Audouin , L , Bacak , M , Balibrea , J , Barbagallo , M , Bečváf , F , Berthoumieux , E , Billowes , J , Bosnar , D , Brown , A , Caamaño , M , Calviño , F , Calviani , M , Cano-Ott , D , Cardella , R , Casanovas , A , Cerutti , F , Chen , Y H , Chiaveri , E , Colonna , N , Cortés , G , Cortés-Giraldo , M A , Cosentino , C , Damone , L A , Diakaki , M , Domingo-Pardo , C , Dressler , L R , Dupont , E , Durán , I , Fernández-Domínguez , B , Ferrari , A , Ferreira , P , Finocchiaro , P , Furman , V , Göbel , K , García , A R , Gawlik , A , Gilardoni , S , Glodariu , T , Gonçalves , I F , González , E , Griesmayer , E , Guerrero , C , Gunsing , F , Harada , H , Heinitz , S , Heyse , J , Jenkins , D G , Jericha , E , Käppeler , F , Kadi , Y , Kalamara , A , Kavrigin , P , Kimura , A , Kivel , N , Kokkoris , M , Krtička , M , Kurtulgil , D , Leal-Cidoncha , E , Lederer , C , Lerendegui-Marco , J , Leeb , H , Lo Meo , S , Lonsdale , S J , Macina , D , Marganiec , J , Martínez , T , Masi , A , Massimi , C , Mastinu , P , Mastromarco , M , Maugeri , E A , Mazzone , A , Mendoza , E , Mengoni , A , Mingrone , F , Milazzo , P M , Musumarra , A , Negret , A , Nolte , R , Oprea , A , Patronis , N , Pavlik , A , Perkowski , J , Porras , I , Praena , J , Quesada , J M , Radeck , D , Rauscher , T , Reifarth , R , Rubbia , C , Ryan , J A , Sabaté-Gilarte , M , Saxena , A , Schillebeeckx , P , Schumann , D , Sedyshev , P , Smith , A G , Sosnin , N V , Stamatopoulos , A , Tain , J L , Tarifeño-Saldivia , A , Tassan-Got , L , Valenta , S , Vannini , G , Variale , V , Vaz , P , Ventura , A , Vlachoudis , V , Vlastou , R , Wallner , A , Warren , S , Woods , P J , Wright , T & Zugec , P 2016 , Recent results in nuclear astrophysics at the n-TOF facility at CERN . in Proceedings of Science . vol. INPC2016 , 161 .
dc.identifier.urihttp://hdl.handle.net/2299/21762
dc.description.abstractThe neutron time of flight (n-TOF) facility at CERN is a spallation source characterized by a white neutron spectrum. The innovative features of the facility, in the two experimental areas, (20 m and 185 m), allow for an accurate determination of the neutron cross section for radioactive samples or for isotopes with small neutron capture cross section, of interest for Nuclear Astrophysics. The recent results obtained at n-TOF facility are presented.en
dc.format.extent499804
dc.language.isoeng
dc.relation.ispartofProceedings of Science
dc.subjectGeneral
dc.titleRecent results in nuclear astrophysics at the n-TOF facility at CERNen
dc.contributor.institutionCentre for Astrophysics Research
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85034616138&partnerID=8YFLogxK
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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