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dc.contributor.authorn TOF Collaboration
dc.contributor.authorLederer-Woods, C.
dc.contributor.authorWoods, P. J.
dc.contributor.authorDavinson, T.
dc.contributor.authorKahl, D.
dc.contributor.authorLonsdale, S. J.
dc.contributor.authorAberle, O.
dc.contributor.authorAmaducci, S.
dc.contributor.authorAndrzejewski, J.
dc.contributor.authorAudouin, L.
dc.contributor.authorBacak, M.
dc.contributor.authorBalibrea, J.
dc.contributor.authorBarbagallo, M.
dc.contributor.authorBečvář, 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, L.
dc.contributor.authorCristallo, S.
dc.contributor.authorDamone, L. A.
dc.contributor.authorDiakaki, M.
dc.contributor.authorDomingo-Pardo, C.
dc.contributor.authorDressler, R.
dc.contributor.authorDupont, E.
dc.contributor.authorDurán, I.
dc.contributor.authorFernández-Domínguez, B.
dc.contributor.authorFerrari, A.
dc.contributor.authorFerreira, P.
dc.contributor.authorFerrer, F. J.
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.authorRauscher, T.
dc.date.accessioned2021-09-13T10:00:03Z
dc.date.available2021-09-13T10:00:03Z
dc.date.issued2021-08-30
dc.identifier.citationn TOF Collaboration , Lederer-Woods , C , Woods , P J , Davinson , T , Kahl , D , Lonsdale , S J , Aberle , O , Amaducci , S , Andrzejewski , J , Audouin , L , Bacak , M , Balibrea , J , Barbagallo , M , Bečvář , 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 , L , Cristallo , S , Damone , L A , Diakaki , M , Domingo-Pardo , C , Dressler , R , Dupont , E , Durán , I , Fernández-Domínguez , B , Ferrari , A , Ferreira , P , Ferrer , F J , Finocchiaro , P , Furman , V , Göbel , K , García , A R , Gawlik , A , Gilardoni , S , Glodariu , T , Gonçalves , I F & Rauscher , T 2021 , ' Destruction of the cosmic γ -ray emitter Al 26 in massive stars: Study of the key Al 26 (n,p) reaction ' , Physical Review C , vol. 104 , no. 2 , L022803 . https://doi.org/10.1103/PhysRevC.104.L022803
dc.identifier.issn2469-9985
dc.identifier.otherPURE: 25928772
dc.identifier.otherPURE UUID: 6ebf3e0d-635f-4c1a-8003-1e6f056f1d2e
dc.identifier.otherScopus: 85114168588
dc.identifier.urihttp://hdl.handle.net/2299/25049
dc.description© 2021 American Physical Society. All rights reserved. Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. https://creativecommons.org/licenses/by/4.0/
dc.description.abstractThe Al26(n,p)Mg26 reaction is the key reaction impacting on the abundances of the cosmic γ-ray emitter Al26 produced in massive stars and impacts on the potential pollution of the early solar system with Al26 by asymptotic giant branch stars. We performed a measurement of the Al26(n,p)Mg26 cross section at the high-flux beam line EAR-2 at the n_TOF facility (CERN). We report resonance strengths for eleven resonances, nine being measured for the first time, while there is only one previous measurement for the other two. Our resonance strengths are significantly lower than the only previous values available. Our cross-section data range to 150 keV neutron energy, which is sufficient for a reliable determination of astrophysical reactivities up to 0.5 GK stellar temperature.en
dc.format.extent7
dc.language.isoeng
dc.relation.ispartofPhysical Review C
dc.subjectNuclear and High Energy Physics
dc.titleDestruction of the cosmic γ -ray emitter Al 26 in massive stars: Study of the key Al 26 (n,p) reactionen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85114168588&partnerID=8YFLogxK
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1103/PhysRevC.104.L022803
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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