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The nucleosynthesis of heavy elements in Stars : The key isotope 25Mg

dc.contributor.authorMassimi, C.
dc.contributor.authorKoehler, P. E.
dc.contributor.authorKopecky, S.
dc.contributor.authorMingrone, F.
dc.contributor.authorSchillebeeckx, P.
dc.contributor.authorVannini, G.
dc.contributor.authorAltstadt, S.
dc.contributor.authorAndrzejewski, J.
dc.contributor.authorAudouin, L.
dc.contributor.authorBarbagallo, M.
dc.contributor.authorBécares, V.
dc.contributor.authorBečvář, F.
dc.contributor.authorBelloni, F.
dc.contributor.authorBerthoumieux, E.
dc.contributor.authorBillowes, J.
dc.contributor.authorBosnar, D.
dc.contributor.authorBrügger, M.
dc.contributor.authorCalviani, M.
dc.contributor.authorCalviño, F.
dc.contributor.authorCano-Ott, D.
dc.contributor.authorCarrapiço, C.
dc.contributor.authorCerutti, F.
dc.contributor.authorChiaveri, E.
dc.contributor.authorChin, M.P.W.
dc.contributor.authorColonna, N.
dc.contributor.authorCortés, G.
dc.contributor.authorCortés-Giraldo, M.A.
dc.contributor.authorDiakaki, M.
dc.contributor.authorDomingo-Pardo, C.
dc.contributor.authorDurán, I.
dc.contributor.authorDressler, R.
dc.contributor.authorEleftheriadis, C.A.
dc.contributor.authorFerrari, A.M.
dc.contributor.authorFraval, K.
dc.contributor.authorGanesan, S.
dc.contributor.authorGarcía, A. R.
dc.contributor.authorGiubrone, G.
dc.contributor.authorGonçalves, I. F.
dc.contributor.authorGonzález-Romero, E.M.
dc.contributor.authorGriesmayer, E.
dc.contributor.authorGuerrero, C.
dc.contributor.authorGunsing, F.
dc.contributor.authorHernández-Prieto, A.
dc.contributor.authorJenkins, D. G.
dc.contributor.authorJericha, E.
dc.contributor.authorKadi, Y.
dc.contributor.authorKäppeler, F.
dc.contributor.authorKaradimos, D.
dc.contributor.authorKivel, N.
dc.contributor.authorKrtička, M.
dc.contributor.authorKroll, J.
dc.contributor.authorLampoudis, C.
dc.contributor.authorLanger, C.
dc.contributor.authorLeal-Cidoncha, E.
dc.contributor.authorLederer, C.
dc.contributor.authorLeeb, H.
dc.contributor.authorLeong, L. S.
dc.contributor.authorLosito, R.
dc.contributor.authorMallick, A.
dc.contributor.authorManousos, A.
dc.contributor.authorMarganiec, J.
dc.contributor.authorMartínez, T.
dc.contributor.authorMastinu, P.F.
dc.contributor.authorMastromarco, M.
dc.contributor.authorMendoza, E.
dc.contributor.authorMengoni, A.
dc.contributor.authorMilazzo, P.M.
dc.contributor.authorMirea, M.
dc.contributor.authorMondalaers, W.
dc.contributor.authorParadela, C.
dc.contributor.authorPavlik, A.
dc.contributor.authorPerkowski, J.
dc.contributor.authorPlompen, A.J.M.
dc.contributor.authorPraena, J.
dc.contributor.authorQuesada, J.M.
dc.contributor.authorRauscher, T.
dc.contributor.authorReifarth, R.
dc.contributor.authorRiego, A.
dc.contributor.authorRobles, M.S.
dc.contributor.authorRubbia, C.
dc.contributor.authorSabaté-Gilarte, M.
dc.contributor.authorSarmento, R.
dc.contributor.authorSaxena, A. C.
dc.contributor.authorSchmidt, S.L.
dc.contributor.authorSchumann, D.L.
dc.contributor.authorTagliente, G.
dc.contributor.authorTaín, J. L.
dc.contributor.authorTarrío, D.
dc.contributor.authorTassan-Got, L.
dc.contributor.authorTsinganis, A.
dc.contributor.authorValenta, S.
dc.contributor.authorVariale, V.
dc.contributor.authorVaz, P.
dc.contributor.authorVentura, A.
dc.contributor.authorVermeulen, M. J.
dc.contributor.authorVlachoudis, V.
dc.contributor.authorVlastou, R.
dc.contributor.authorWallner, A.
dc.contributor.authorWare, T.
dc.contributor.authorWeigand, M.
dc.contributor.authorWeiss, C.
dc.contributor.authorWright, T. J.
dc.contributor.authorŽugec, P.
dc.date.accessioned2014-05-29T12:30:24Z
dc.date.available2014-05-29T12:30:24Z
dc.date.issued2014-04-14
dc.identifier.citationMassimi , C , Koehler , P E , Kopecky , S , Mingrone , F , Schillebeeckx , P , Vannini , G , Altstadt , S , Andrzejewski , J , Audouin , L , Barbagallo , M , Bécares , V , Bečvář , F , Belloni , F , Berthoumieux , E , Billowes , J , Bosnar , D , Brügger , M , Calviani , M , Calviño , F , Cano-Ott , D , Carrapiço , C , Cerutti , F , Chiaveri , E , Chin , M P W , Colonna , N , Cortés , G , Cortés-Giraldo , M A , Diakaki , M , Domingo-Pardo , C , Durán , I , Dressler , R , Eleftheriadis , C A , Ferrari , A M , Fraval , K , Ganesan , S , García , A R , Giubrone , G , Gonçalves , I F , González-Romero , E M , Griesmayer , E , Guerrero , C , Gunsing , F , Hernández-Prieto , A , Jenkins , D G , Jericha , E , Kadi , Y , Käppeler , F , Karadimos , D , Kivel , N , Krtička , M , Kroll , J , Lampoudis , C , Langer , C , Leal-Cidoncha , E , Lederer , C , Leeb , H , Leong , L S , Losito , R , Mallick , A , Manousos , A , Marganiec , J , Martínez , T , Mastinu , P F , Mastromarco , M , Mendoza , E , Mengoni , A , Milazzo , P M , Mirea , M , Mondalaers , W , Paradela , C , Pavlik , A , Perkowski , J , Plompen , A J M , Praena , J , Quesada , J M , Rauscher , T , Reifarth , R , Riego , A , Robles , M S , Rubbia , C , Sabaté-Gilarte , M , Sarmento , R , Saxena , A C , Schmidt , S L , Schumann , D L , Tagliente , G , Taín , J L , Tarrío , D , Tassan-Got , L , Tsinganis , A , Valenta , S , Variale , V , Vaz , P , Ventura , A , Vermeulen , M J , Vlachoudis , V , Vlastou , R , Wallner , A , Ware , T , Weigand , M , Weiss , C , Wright , T J & Žugec , P 2014 , ' The nucleosynthesis of heavy elements in Stars : The key isotope 25Mg ' , EPJ Web of Conferences , vol. 66 , 07016 . https://doi.org/10.1051/epjconf/20146607016
dc.identifier.issn2101-6275
dc.identifier.urihttp://hdl.handle.net/2299/13578
dc.descriptionThis is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited
dc.description.abstractWe have measured the radiative neutron-capture cross section and the total neutron-induced cross section of one of the most important isotopes for the s process, the 25Mg. The measurements have been carried out at the neutron time-of-flight facilities n-TOF at CERN (Switzerland) and GELINA installed at the EC-JRC-IRMM (Belgium). The cross sections as a function of neutron energy have been measured up to approximately 300 keV, covering the energy region of interest to the s process. The data analysis is ongoing and preliminary results show the potential relevance for the s process.en
dc.format.extent4
dc.format.extent407170
dc.language.isoeng
dc.relation.ispartofEPJ Web of Conferences
dc.titleThe nucleosynthesis of heavy elements in Stars : The key isotope 25Mgen
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.versionofrecord10.1051/epjconf/20146607016
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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