no code implementations • 20 Jun 2018 • Mikhail V. Beznogov, Ermal Rrapaj, Dany Page, Sanjay Reddy
If the thermal evolution of the hot young neutron star in the supernova remnant HESS J1731-347 is driven by neutrino emission, it provides a stringent constraint on the coupling of light (mass $\ll 10$ keV) axion-like particles to neutrons.
High Energy Astrophysical Phenomena
