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Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/849
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dc.contributor.authorAbgrall, N.en
dc.contributor.authorAduszkiewicz, A.en
dc.contributor.authorAnticic, T.en
dc.contributor.authorAntoniou, N.en
dc.contributor.authorArgyriades, J.en
dc.contributor.authorBaatar, B.en
dc.contributor.authorBlondel, A.en
dc.contributor.authorBlumer, J.en
dc.contributor.authorBogomilov, M.en
dc.contributor.authorBravar, A.en
dc.contributor.authorBrooks, W.en
dc.contributor.authorBrzychczyk, J.en
dc.contributor.authorBubak, A.en
dc.contributor.authorBunyatov, S. A.en
dc.contributor.authorBusygina, O.en
dc.contributor.authorChristakoglou, P.en
dc.contributor.authorChung, P.en
dc.contributor.authorCzopowicz, T.en
dc.contributor.authorDavis, N.en
dc.contributor.authorDebieux, S.en
dc.contributor.authorDi Luise, S.en
dc.contributor.authorDominik, W.en
dc.contributor.authorDumarchez, J.en
dc.contributor.authorDynowski, K.en
dc.contributor.authorEngel, R.en
dc.contributor.authorEreditato, A.en
dc.contributor.authorEsposito, L. S.en
dc.contributor.authorFeofilov, G. A.en
dc.contributor.authorFodor, Z.en
dc.contributor.authorFerrero, A.en
dc.contributor.authorFulop, A.en
dc.contributor.authorGaździcki, M.en
dc.contributor.authorGolubeva, M.en
dc.contributor.authorGrabez, B.en
dc.contributor.authorGrebieszkow, K.en
dc.contributor.authorGrzeszczuk, A.en
dc.contributor.authorGuber, F.en
dc.contributor.authorHaesler, A.en
dc.contributor.authorHakobyan, H.en
dc.contributor.authorHasegawa, T.en
dc.contributor.authorIdczak, R.en
dc.contributor.authorIgolkin, S.en
dc.contributor.authorIvanov, Y.en
dc.contributor.authorIvashkin, A.en
dc.contributor.authorKadija, K.en
dc.contributor.authorKapoyannis, A.en
dc.contributor.authorKatryńska, N.en
dc.contributor.authorKiełczewska, D.en
dc.contributor.authorKikola, D.en
dc.contributor.authorKirejczyk, M.en
dc.contributor.authorKisiel, J.en
dc.contributor.authorKiss, T.en
dc.contributor.authorKleinfelder, S.en
dc.contributor.authorKobayashi, T.en
dc.contributor.authorKochebina, O.en
dc.contributor.authorKolesnikov, V. I.en
dc.contributor.authorKolev, D.en
dc.contributor.authorKondratiev, V. P.en
dc.contributor.authorKorzenev, A.en
dc.contributor.authorKowalski, S.en
dc.contributor.authorKrasnoperov, A.en
dc.contributor.authorKuleshov, S.en
dc.contributor.authorKurepin, A.en
dc.contributor.authorLacey, R.en
dc.contributor.authorLarsen, D.en
dc.contributor.authorLaszlo, A.en
dc.contributor.authorLyubushkin, V. V.en
dc.contributor.authorMaćkowiak-Pawłowska, M.en
dc.contributor.authorMajka, Z.en
dc.contributor.authorMaksiak, B.en
dc.contributor.authorMalakhov, A. I.en
dc.contributor.authorMaletic, D.en
dc.contributor.authorMarchionni, A.en
dc.contributor.authorMarcinek, A.en
dc.contributor.authorMaris, I.en
dc.contributor.authorMarin, V.en
dc.contributor.authorMarton, K.en
dc.contributor.authorMatulewicz, T.en
dc.contributor.authorMatveev, V.en
dc.contributor.authorMelkumov, G. L.en
dc.contributor.authorMessina, M.en
dc.contributor.authorMrówczyński, Sten
dc.contributor.authorMurphy, S.en
dc.contributor.authorNakadaira, T.en
dc.contributor.authorNishikawa, K.en
dc.contributor.authorPalczewski, T.en
dc.contributor.authorPalla, G.en
dc.contributor.authorPanagiotou, A. D.en
dc.contributor.authorPaul, T.en
dc.contributor.authorPeryt, W.en
dc.contributor.authorPetukhov, O.en
dc.contributor.authorPłaneta, R.en
dc.contributor.authorPluta, J.en
dc.contributor.authorPopov, B. A.en
dc.contributor.authorPosiadała, M.en
dc.contributor.authorPuławski, S.en
dc.contributor.authorPuzović, Jovanen
dc.contributor.authorRauch, W.en
dc.contributor.authorRavonel, M.en
dc.contributor.authorRenfordt, R.en
dc.date.accessioned2022-07-12T17:16:53Z-
dc.date.available2022-07-12T17:16:53Z-
dc.date.issued2013-02-11en
dc.identifier.issn0168-9002en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/849-
dc.description.abstractThe T2K long-baseline neutrino oscillation experiment in Japan needs precise predictions of the initial neutrino flux. The highest precision can be reached based on detailed measurements of hadron emission from the same target as used by T2K exposed to a proton beam of the same kinetic energy of 30 GeV. The corresponding data were recorded in 2007–2010 by the NA61/SHINE experiment at the CERN SPS using a replica of the T2K graphite target. In this paper details of the experiment, data taking, data analysis method and results from the 2007 pilot run are presented. Furthermore, the application of the NA61/SHINE measurements to the predictions of the T2K initial neutrino flux is described and discussed.en
dc.relation.ispartofNuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipmenten
dc.subjectHadron productionen
dc.subjectLong targeten
dc.subjectNeutrino flux predictionsen
dc.titlePion emission from the T2K replica target: Method, results and applicationen
dc.typeArticleen
dc.identifier.doi10.1016/j.nima.2012.10.079en
dc.identifier.scopus2-s2.0-84869885392en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84869885392en
dc.relation.volume701en
dc.relation.firstpage99en
dc.relation.lastpage114en
item.grantfulltextnone-
item.openairetypeArticle-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
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