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Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/1316
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dc.contributor.authorAmin, Neerajen
dc.contributor.authorAcharya, A.en
dc.contributor.authorAdhikary, H.en
dc.contributor.authorAllison, K. K.en
dc.contributor.authorAndronov, E. V.en
dc.contributor.authorAntićić, T.en
dc.contributor.authorBabkin, V.en
dc.contributor.authorBaszczyk, M.en
dc.contributor.authorBhosale, S.en
dc.contributor.authorBlondel, A.en
dc.contributor.authorBogomilov, M.en
dc.contributor.authorBondar, Y.en
dc.contributor.authorBrandin, A.en
dc.contributor.authorBravar, A.en
dc.contributor.authorBryliński, W.en
dc.contributor.authorBrzychczyk, J.en
dc.contributor.authorBuryakov, M.en
dc.contributor.authorBusygina, O.en
dc.contributor.authorCherif, H.en
dc.contributor.authorĆirković, Marjanen
dc.contributor.authorCsanad, M.en
dc.contributor.authorCybowska, J.en
dc.contributor.authorCzopowicz, T.en
dc.contributor.authorDamyanova, A.en
dc.contributor.authorDavis, N.en
dc.contributor.authorDeveaux, M.en
dc.contributor.authorDmitriev, A.en
dc.contributor.authorDominik, W.en
dc.contributor.authorDorosz, P.en
dc.contributor.authorDumarchez, J.en
dc.contributor.authorEngel, R.en
dc.contributor.authorFeofilov, G. A.en
dc.contributor.authorFields, L.en
dc.contributor.authorFodor, Z.en
dc.contributor.authorGaribov, A.en
dc.contributor.authorGaździcki, M.en
dc.contributor.authorGolosov, O.en
dc.contributor.authorGolovatyuk, V.en
dc.contributor.authorGolubeva, M.en
dc.contributor.authorGrebieszkow, K.en
dc.contributor.authorGuber, F.en
dc.contributor.authorHaesler, A.en
dc.contributor.authorIgolkin, S. N.en
dc.contributor.authorIlieva, S.en
dc.contributor.authorIvashkin, A.en
dc.contributor.authorJohnson, S. R.en
dc.contributor.authorKadija, K.en
dc.contributor.authorKargin, N.en
dc.contributor.authorKashirin, E.en
dc.contributor.authorKiełbowicz, M.en
dc.contributor.authorKireyeu, V. A.en
dc.contributor.authorKlochkov, V.en
dc.contributor.authorKolesnikov, V. I.en
dc.contributor.authorKolev, D.en
dc.contributor.authorKorzenev, A.en
dc.contributor.authorKovalenko, V. N.en
dc.contributor.authorKowalski, S.en
dc.contributor.authorKoziel, M.en
dc.contributor.authorKozłowski, B.en
dc.contributor.authorKrasnoperov, A.en
dc.contributor.authorKucewicz, W.en
dc.contributor.authorKuich, M.en
dc.contributor.authorKurepin, A.en
dc.contributor.authorLarsen, D.en
dc.contributor.authorLászló, A.en
dc.contributor.authorLazareva, T. V.en
dc.contributor.authorLewicki, M.en
dc.contributor.authorŁojek, K.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.authorMarcinek, A.en
dc.contributor.authorMarino, A. D.en
dc.contributor.authorMarton, K.en
dc.contributor.authorMathes, H. J.en
dc.contributor.authorMatulewicz, T.en
dc.contributor.authorMatveev, V.en
dc.contributor.authorMelkumov, G. L.en
dc.contributor.authorMerzlaya, A. O.en
dc.contributor.authorMesserly, B.en
dc.contributor.authorMiken
dc.contributor.authorMorozov, S.en
dc.contributor.authorNagai, Y.en
dc.contributor.authorNaskręt, M.en
dc.contributor.authorOzvenchuk, V.en
dc.contributor.authorPanova, O.en
dc.contributor.authorPaolone, V.en
dc.contributor.authorPetukhov, O.en
dc.contributor.authorPidhurskyi, I.en
dc.contributor.authorPłaneta, R.en
dc.contributor.authorPodlaski, P.en
dc.contributor.authorPopov, B. A.en
dc.contributor.authorPorfy, B.en
dc.contributor.authorPosiadała-Zezula, M.en
dc.contributor.authorProkhorova, D. S.en
dc.contributor.authorPszczel, D.en
dc.contributor.authorPuławski, S.en
dc.contributor.authorPuzović, Jovanen
dc.date.accessioned2023-03-08T10:34:02Z-
dc.date.available2023-03-08T10:34:02Z-
dc.date.issued2022-03-18en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/1316-
dc.description.abstractWe report the analysis of data taken during a pilot run in 2018 to study the feasibility of nuclear fragmentation measurements with the NA61/SHINE experiment at the CERN SPS. These nuclear reactions are important for the interpretation of secondary cosmic-ray nuclei production (Li, Be, and B) in the Galaxy. The pilot data were taken with 12C projectiles at a beam momentum of 13.5 AGeV/c and two fixed targets, polyethylene (C2H4) and graphite. The specific focus here is the measurement of total Boron (10B and 11B) production cross section in C+p interactions at 13.5 AGeV/c. The cosmic-ray nucleus 11C is termed a ‘Ghost nucleus’ on account of its short lifetime compared to the usual cosmic-ray diffusion time in the Galaxy and it ultimately decays to Boron as, 11C → 11B + β+. Therefore, precise knowledge of the production cross section of 11C is very relevant for the understanding of Boron production in the Galaxy. We present a preliminary measurement of the fragmentation cross section of C + p → 11C, which, together with our previously reported B-production cross section, provides a new constraint on boron production in the Galaxy in the high-energy range relevant for modern space based cosmic-ray experiments like AMS-02.en
dc.relation.ispartofProceedings of Scienceen
dc.titleResults from a Pilot Study on the Measurement of Nuclear Fragmentation with NA61/SHINE at the CERN SPS: <sup>11</sup>C Production in C+p Interactions at 13.5 AGeV/cen
dc.typeConference Paperen
dc.identifier.scopus2-s2.0-85145006384en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85145006384en
dc.relation.volume395en
item.openairetypeConference Paper-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.orcid0000-0002-4420-9688-
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