A gamma-ray signature of energetic sources of cosmic-ray nuclei

Details A gamma-ray signature of energetic sources of cosmic-ray nuclei A gamma-ray signature of energetic sources of cosmic-ray nuclei

2011-09-02

arxiv.org/abs/1109.0565v3

Physics Letters B 707, 255 (2012)

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

10 pages, 3 figures; final draft accepted for publication

Scientific paper

10.1016/j.physletb.2011.12.045

Astrophysical sources of nuclei are expected to produce a broad spectrum of isotopes, many of which are unstable. An unstable nucleus can beta-decay outside the source into a single-electron ion. Heavy one-electron ions, thus formed, can be excited in their interactions with cosmic microwave background photons, in which case they relax to the ground state with the emission of a gamma ray. Repetitive cycles of excitation and gamma-ray emission can produce an observable feature in the gamma-ray spectrum with a maximum around 8 GeV (for iron). We find that the observed spectrum of Centaurus A is consistent with a substantial flux of nuclei accelerated to 0.1 EeV. A characteristic 5--10 GeV (iron) shoulder in the gamma-ray spectra of various sources can help identify astrophysical accelerators of nuclei or set upper limits on nuclear acceleration.

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