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EBL Inhomogeneity and Hard-Spectrum Gamma-Ray Sources

  • Authors: Hassan Abdalla, and Markus Böttcher

2017 The Astrophysical Journal 835 237.

  • Provider: AAS Journals

Caption: Figure 3.

Top panels: differential EBL photon energy density as a function of distance along the line of sight for various sizes (as indicated by the labels) of a void located at zv = 0.5 at two representative photon energies of ϵ = 1 eV (left) and ϵ = 8 eV (right). The red solid lines (R = 0) represent the homogeneous case. The general increase of the EBL energy density with redshift is due to the ﹩{(1+{z}_{1})}^{4}﹩ factor in Equation (5) and the increase in star formation rate with redshift. Bottom panels: relative EBL energy density deficit due to the presence of a void for the same cases as in the top panels. The red vertical lines indicate the boundaries of the void for the R = 100 h−1 Mpc case.

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