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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 4.

Left panel: relative differential EBL energy density deficit as a function of distance along the line of sight for various EBL photon energy densities in the case of an R = 50 h−1 Mpc void located at zv = 0.5. The red vertical lines indicate the boundaries of the void. Right panel: angle dependence (θ is the angle with respect to the direct line of sight through the center of the void) of the EBL energy density in the presence of an R = 50 h−1 Mpc at the zv = 0.5 void (dashed lines), compared to the homogeneous case (which does not have any angle dependence; solid lines), at a representative near-UV photon energy of ϵ = 8 eV for three positions (redshifts) along the line of sight: at the center of the void (black, lower curves), within the void but behind its center (red curves), and behind the void (blue and cyan, upper curves).

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