Gamma ray astronomy and the origin of the light nuclei

Physics – Nuclear Physics

Scientific paper

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Cosmic Rays, Gamma Ray Astronomy, Interstellar Gas, Light Elements, Nuclear Particles, Nuclei (Nuclear Physics), Abundance, Beryllium Isotopes, Boron Isotopes, Continuous Spectra, Energy Spectra, Lithium Isotopes

Scientific paper

Nuclear reactions induced by the collisions of the protons and alphas of the galactic cosmic ray with heavy nuclei of the interstellar gas are responsible for the continuous production of the light elements lithium, beryllium, and boron in the galaxy. To better than one order of magnitude, the observed ratios of these abundances to hydrogen abundance and the nuclidic abundance ratios between themselves are accounted for by simply considering the effect of fast protons and alphas with a flux and an energy spectrum as observed in galactic cosmic rays, for a period comparable with the life of our galaxy. The role of gamma ray astronomy in solving problems that occur when accurate agreement is sought with increasingly accurate data is discussed.

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