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U(n,f) cross section from n_TOF (CERN) from 18 meV to 10 keV

dc.contributor.authorMastromarco, M.
dc.contributor.authorAmaducci, S.
dc.contributor.authorColonna, N.
dc.contributor.authorFinocchiaro, P.
dc.contributor.authorCosentino, L.
dc.contributor.authorBarbagallo, M.
dc.contributor.authorAberle, O.
dc.contributor.authorAndrzejewski, J.
dc.contributor.authorAudouin, L.
dc.contributor.authorBacak, M.
dc.contributor.authorBalibrea, J.
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.authorCortés, G.
dc.contributor.authorCortés-Giraldo, M. A.
dc.contributor.authorDamone, L. A.
dc.contributor.authorDiakaki, M.
dc.contributor.authorDomingo-Pardo, C.
dc.contributor.authorDiacono, D.
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.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-Romero, 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.authorKnapova, I.
dc.contributor.authorKokkoris, M.
dc.contributor.authorKrtička, M.
dc.contributor.authorKurtulgil, D.
dc.contributor.authorLeal-Cidoncha, E.
dc.contributor.authorLederer, C.
dc.contributor.authorLeeb, H.
dc.contributor.authorLerendegui-Marco, J.
dc.contributor.authorMeo, S. Lo
dc.contributor.authorLonsdale, S. J.
dc.contributor.authorMacina, D.
dc.contributor.authorManna, A.
dc.contributor.authorMarganiec, J.
dc.contributor.authorMartínez, T.
dc.contributor.authorMasi, A.
dc.contributor.authorMassimi, C.
dc.contributor.authorMastinu, P.
dc.contributor.authorMaugeri, E. A.
dc.contributor.authorMazzone, A.
dc.contributor.authorMendoza, E.
dc.contributor.authorMengoni, A.
dc.contributor.authorMilazzo, P. M.
dc.contributor.authorMingrone, F.
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.authorTagliente, G.
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.authorWeiss, C.
dc.contributor.authorWoods, P. J.
dc.contributor.authorWright, T.
dc.contributor.authorŽugec, P.
dc.date.accessioned2023-11-27T00:34:03Z
dc.date.available2023-11-27T00:34:03Z
dc.date.issued2022-08-13
dc.date.updated2022-08-14T10:05:46Z
dc.description.abstractThe 235U(n,f) cross section was measured in a wide energy range (18 meV–170 keV) at the n_TOF facility at CERN, relative to 6Li(n,t) and 10B(n,α) standard reactions, with high resolution and accuracy, with a setup based on a stack of six samples and six silicon detectors placed in the neutron beam. In this paper we report on the results in the region between 18 meV and 10 keV neutron energy. A resonance analysis has been performed up to 200 eV, with the code SAMMY. The resulting fission kernels are compared with the ones extracted on the basis of the resonance parameters of the most recent major evaluated data libraries. A comparison of the n_TOF data with the evaluated cross sections is also performed from thermal to 10 keV neutron energy for the energy-averaged cross section in energy groups of suitably chosen width. A good agreement, within 0.5%, is found on average between the new results and the latest evaluated data files ENDF/B-VIII.0 and JEFF-3.3, as well as with respect to the broad group average fission cross section established in the framework of the standard working group of IAEA (the so-called reference file). However, some discrepancies, of up to 4%, are still present in some specific energy regions. The new dataset here presented, characterized by a unique combination of high resolution and accuracy, low background and wide energy range, can help to improve the evaluations from the Resolved Resonance Region up to 10 keV, also reducing the uncertainties that affect this region.en_AU
dc.description.sponsorshipOpen access funding provided by CERN (European Organization for Nuclear Research).en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn1434-601Xen_AU
dc.identifier.urihttp://hdl.handle.net/1885/307439
dc.language.isoen_AUen_AU
dc.provenanceThis article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecomm ons.org/licenses/by/4.0/.en_AU
dc.publisherSpringer Berlin Heidelbergen_AU
dc.rights© The Author(s) 2022en_AU
dc.rights.licenseCreative Commons Attribution Licenseen_AU
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_AU
dc.sourceThe European Physical Journal Aen_AU
dc.titleU(n,f) cross section from n_TOF (CERN) from 18 meV to 10 keVen_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue8en_AU
local.bibliographicCitation.lastpage147-13en_AU
local.bibliographicCitation.startpage147-1en_AU
local.contributor.affiliationWallner, A., The Australian National Universityen_AU
local.description.notesImported from Springer Natureen_AU
local.identifier.citationvolume58en_AU
local.identifier.doi10.1140/epja/s10050-022-00779-7en_AU
local.publisher.urlhttps://link.springer.com/en_AU
local.type.statusPublished Versionen_AU

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