Axion-photon multimessenger astronomy with giant flares
arXiv:2201.04059 · doi:10.1103/PhysRevD.106.L041302
Abstract
We treat prospects for multimessenger astronomy with giant flares (GFs), a rare transient event featured by magnetars that can be as luminous as a hundred of the brightest supernovae ever observed. The beamed photons could correlate with an axion counterpart via resonant conversion in the magnetosphere. In a realistic parameter space, we find that the sensitivity limit to galactic GFs for currently viable experiments is GeV \& . We rule out the compatibility of axion flares with the recent XENON1T excess only due to the time persistence of the signal.
arXiv comment7 pages, 3 figures
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