New solar X-ray constraints on keV Axion-Like Particles

Abstract

The decay of Axion-Like Particles (ALPs) trapped in the solar gravitational field would contribute to the observed solar X-ray flux, hence constraining ALP models. We improve by one order of magnitude the existing limits in the parameter space $(g_{a\gamma \gamma },m)$ by considering ALPs production via photon coalescence. For $g_{ae}\ne 0$, we demonstrate that trapped ALPs can be Compton-absorbed while crossing the Sun, resulting in two regimes in the exclusion limits, with a transition triggered by $g_{ae}$. Out of the transitional region, the solar X-ray constraints on ALPs are exclusively governed by $g_{a\gamma \gamma }$.

Comments: 6 pages, 4 figures