1 code implementation • 27 Aug 2019 • Collin D. Capano, Ingo Tews, Stephanie M. Brown, Ben Margalit, Soumi De, Sumit Kumar, Duncan A. Brown, Badri Krishnan, Sanjay Reddy
The properties of neutron stars are determined by the nature of the matter that they contain.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology High Energy Physics - Phenomenology Nuclear Theory
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