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The results of ATIC-2 experiment for elemental spectra of cosmic rays

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arxiv astro-ph/0612377 v1 pith:HAQCNEKD submitted 2006-12-14 astro-ph

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keywords protonsspectranucleiatic-2cosmicenergyexperimentrays
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The results of ATIC-2 baloon experiment (2002-2003) for energy spectra of protons, He, C, O, Ne, Mg, Si, Fe, some groups of nuclei, and all-particle spectrum in primary cosmic rays are presented in energy region 50GeV--200TeV. The conclusion is that the spectra of protons and helium nuclei are essentially different (the spectrum of protons is steeper) and the spectra of protons and heavy nuclei have no-power form.

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  1. Deciphering the spectral bumps of Galactic cosmic rays through gamma-ray observations of nearby molecular clouds

    astro-ph.HE 2025-01 conditional novelty 6.0 of 10

    A nearby cosmic-ray source would make the gamma-ray spectral indices of molecular clouds evolve differently with energy, providing a new observational test.

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