In a Galactic core-collapse supernova (SN), axionlike particles (ALPs) could be emitted via the Primakoff process and eventually convert into γ rays in the magnetic field of the Milky Way. From a data-driven sensitivity estimate, we find that, for a SN exploding in our Galaxy, the Fermi Large Area Telescope (LAT) would be able to explore the photon-ALP coupling down to gaγ≃2×10−13GeV−1 for an ALP mass ma≲10−9eV. These values are out of reach of next generation laboratory experiments. In this event, the Fermi LAT would probe large regions of the ALP parameter space invoked to explain the anomalous transparency of the Universe to γ rays, stellar cooling anomalies, and cold dark matter. If no γ-ray emission were to be detected, Fermi-LAT observations would improve current bounds derived from SN1987A by more than one order of magnitude.
@article{arxiv.1609.02350,
title = {The Fermi Large Area Telescope as a Galactic Supernovae Axionscope},
author = {Manuel Meyer and Maurizio Giannotti and Alessandro Mirizzi and Jan Conrad and Miguel Sanchez-Conde},
journal= {arXiv preprint arXiv:1609.02350},
year = {2017}
}