Hunting Dark Matter with Gamma Rays

A simulated flux realization of Mrk 501, modeled across 25 logarithmically-spaced energy bins, demonstrates how the best-fit ECPL function [latex]H_0[/latex] is altered by the attenuation effect of dark photon scattering-specifically for a dark photon with a coupling of [latex]A^{\prime} = 1~\mathrm{eV}[/latex] and mixing parameter of [latex]\varepsilon = 5 \times 10^{-8}[/latex]-as detailed in Table 3.

A new study explores how the Cherenkov Telescope Array could reveal the presence of dark photon dark matter by observing subtle distortions in high-energy light from distant sources.