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THE ORIGIN OF THE COSMIC GAMMA-RAY BACKGROUND IN THE MeV RANGE

  • Authors: Pilar Ruiz-Lapuente, Lih-Sin The, Dieter H. Hartmann, Marco Ajello, Ramon Canal, Friedrich K. Röpke, Sebastian T. Ohlmann, and Wolfgang Hillebrandt

2016 The Astrophysical Journal 820 142.

  • Provider: AAS Journals

Caption: Figure 10.

Gamma-ray background using the Graur et al. (2014) compilation of SN Ia rates (solid line; see Figures 5 and 6), and the upper 1σ (blue dashed line) and 2σ bounds (red dotted line). With those rates, the SNe Ia cannot account for the observed gamma-ray background at the 2σ level (nor even at the 3σ level). The model used is the fully mixed W7 (W99b), but predictions for the other models are qualitatively similar.

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