EBL Inhomogeneity and Hard-Spectrum Gamma-Ray Sources

被引：11

作者：

Abdalla, Hassan ^{[1
,2
]}

Bottcher, Markus ^{[1
]}

机构：

[1] North West Univ, Ctr Space Res, ZA-2520 Potchefstroom, South Africa

[2] Omdurman Islamic Univ, Dept Astron & Meteorol, Omdurman 382, Sudan

来源：

ASTROPHYSICAL JOURNAL | 2017年 / 835卷 / 02期

基金：

新加坡国家研究基金会;

关键词：

cosmology: miscellaneous; galaxies: active; galaxies: jets; radiation mechanisms: non-thermal; EXTRAGALACTIC BACKGROUND LIGHT; ABSORPTION; RADIATION; ORIGIN;

D O I：

10.3847/1538-4357/835/2/237

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The unexpectedly hard very-high-energy (VHE; E > 100 GeV) gamma-ray spectra of a few distant blazars have been interpreted as evidence of a reduction of the gamma gamma opacity of the universe due to the interaction of VHE gamma-rays with the extragalactic background light (EBL) compared to the expectation from current knowledge of the density and cosmological evolution of the EBL. One of the suggested solutions to this problem involves the inhomogeneity of the EBL. In this paper, we study the effects of such inhomogeneity on the energy density of the EBL (which then also becomes anisotropic) and the resulting gamma gamma opacity. Specifically, we investigate the effects of cosmic voids along the line of sight to a distant blazar. We find that the effect of such voids on the gamma gamma opacity, for any realistic void size, is only of the order of less than or similar to 1 % and much smaller than expected from a simple linear scaling of the gamma gamma opacity with the line-of-sight galaxy underdensity due to a cosmic void.

引用

页数：8

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