Add to ORKGAccurate evaluation of production cross sections of light elements is impor-tant for models of CR propagation, galactic chemical evolution, and cosmological studies. However, experimental spallation cross section data are scarce and often unavailable to CR community while semi-empirical systematics are frequently wrong by a significant factor. We use all available data from LANL nuclear database together with modern nuclear codes to produce evaluated production cross sections of isotopes of Li, Be, B suitable for astrophysical applications. 1
International audienceContext. We reassess the problem of the production and evolution of the light ...
Context. We reassess the problem of the production and evolution of the light elements Li,...
Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-...
The precision of the current generation of cosmic-ray (CR) experiments, such as AMS-02, PAMELA, CALE...
International audienceHigh-precision cosmic-ray data from ongoing and recent past experiments (Voyag...
Les isotopes de Li, Be, B tiennent une place particulière dans la répartition des éléments. On discu...
The origin and evolution of isotopes of the lightest elements H2, He3, Li, Be, B in the universe is ...
Abstract: Last several years were rich with discoveries in astrophysics of cosmic rays (CRs), thanks...
7 pages, 2 figures - Proceeding of the 34th International Cosmic Ray ConferenceInternational audienc...
Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise und...
13 pages, 12 figures, 4 tables. Accepted by ApJMeasurement of the chemical and isotopic composition ...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCR) between E=50-200 MeV/nucleon h...
Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise und...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCRs) between E = 50 and 200 MeV/nu...
International audienceContext. We reassess the problem of the production and evolution of the light ...
Context. We reassess the problem of the production and evolution of the light elements Li,...
Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-...
The precision of the current generation of cosmic-ray (CR) experiments, such as AMS-02, PAMELA, CALE...
International audienceHigh-precision cosmic-ray data from ongoing and recent past experiments (Voyag...
Les isotopes de Li, Be, B tiennent une place particulière dans la répartition des éléments. On discu...
The origin and evolution of isotopes of the lightest elements H2, He3, Li, Be, B in the universe is ...
Abstract: Last several years were rich with discoveries in astrophysics of cosmic rays (CRs), thanks...
7 pages, 2 figures - Proceeding of the 34th International Cosmic Ray ConferenceInternational audienc...
Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise und...
13 pages, 12 figures, 4 tables. Accepted by ApJMeasurement of the chemical and isotopic composition ...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCR) between E=50-200 MeV/nucleon h...
Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise und...
The abundance of Li, Be, and B isotopes in galactic cosmic rays (GCRs) between E = 50 and 200 MeV/nu...
International audienceContext. We reassess the problem of the production and evolution of the light ...
Context. We reassess the problem of the production and evolution of the light elements Li,...
Precise measurements of predominantly secondary cosmic-ray Li, Be, and B together with current well-...