We show that solar γ-ray observations can provide a complementary
probe of Dark Matter in scenarios where the interactions with the Standard
Model proceed via long-lived mediators. For illustration we consider a
simplified model which provides solar γ-ray fluxes observable with the
next generation γ-ray telescopes, while complying with the existing
experimental constraints. Our results suggest that solar γ-ray fluxes
can be orders of magnitude larger than the ones from the Galactic center, while
being subject to low backgrounds.Comment: 4 pages, 2 figures. To appear in the proceedings of The European
Physical Society Conference on High Energy Physics, 5-12 July 2017 in Venice,
Ital