NSR Query Results
Output year order : Descending NSR database version of May 10, 2024. Search: Author = D.Maurin Found 1 matches. 2018GE07 Phys.Rev. C 98, 034611 (2018) Y.Genolini, D.Maurin, I.V.Moskalenko, M.Unger Current status and desired precision of the isotopic production cross sections relevant to astrophysics of cosmic rays: Li, Be, B, C, and N NUCLEAR REACTIONS 1H(10B, X), (11B, X)6Li/7Li/9Li/7Be/9Be/10Be/10B, E=0.1-10 GeV/nucleon; 1H(12C, X), (13C, X)6Li/7Li/9Li/7Be/9Be/10Be/10B/11B/10C/11C, E=0.1-10 GeV/nucleon; 1H(14N, X), (15N, X)6Li/7Li/9Li/7Be/9Be/10Be/10B/11B/11C/12C/13C/14C/12N/13N/14N, E=0.1-10 GeV/nucleon; 1H(16O, X)6Li/7Li/9Li/7Be/9Be/10Be/12Be/10B/11B/12B/12C/13C/14C/12N/13N/14N/15N/13O/14O/15O, E=0.1-10 GeV/nucleon; 1H(20Ne, X), (21Ne, X), (22Ne, X)10B/11B/12B/10C/11C/12C/13C/14C/15C/12N/13N/14N/15N/14O/15O/16O/18F/19F/19Ne, E=0.1-10 GeV/nucleon; 1H(23Na, X)15O/16O/19F, E=0.1-10 GeV/nucleon; 1H(24Mg, X), (25Mg, X), (26Mg, X)10B/11B/12B/11C/12C/13C/14C/15C/16C/12N/13N/14N/15N/14O/15O/16O/18F/19F/19Ne/20Ne/21Ne/22Ne/22Na/23Na/23Mg, E=0.1-10 GeV/nucleon; 1H(27Al, X)15O/19F, E=0.1-10 GeV/nucleon; 1H(28Si, X), (29Si, X)9Be/15O/16O/19F/19Ne/20Ne/22Na/24Mg/27Al/27Si, E=0.1-10 GeV/nucleon; 1H(56Fe, X), 39Ar/40K/41K/44Sc/45Sc, E=0.1-10 GeV/nucleon; analyzed production σ(E) with benchmark parametrizations and compared with experimental data for the most important reaction channels for production of most astrophysically important isotopes of Li, Be, B, C, and N in cosmic ray interactions; deduced ranking of the reaction channels by their importance for a production of a particular isotope. See Supplemental Material of this paper on 52 pages for an extensive list of relevant reactions, irrespective of their flux impact on cosmic rays. Relevance to high precision modern generation cosmic-ray (CR) experiments such as AMS-02, PAMELA, CALET, ISS-CREAM, BESS-Polar, and Fermi-LAT.
doi: 10.1103/PhysRevC.98.034611
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