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Search: Author = I.V.Moskalenko

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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
Citations: PlumX Metrics

1989MO16      Yad.Fiz. 49, 1623 (1989)

I.V.Moskalenko, O.V.Fotina

Energy Spectrum of γ Quanta from Giant Dipole Resonance Decay in Iron

NUCLEAR REACTIONS ⁵⁶Fe(γ, n), E=10-25 MeV; calculated σ(E). ⁵⁶Fe(γ, xγ), E=10-25 MeV; calculated Eγ, Iγ, mean γ-multiplicity. Statistical theory.