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Beamed emission from a neutron-star ULX in a GRRMHD simulation

By David Abarca and others
We perform a global 2.5D general-relativistic radiation magnetohydrodynamic simulation of super-critical accretion onto a neutron star with a 2×10102\times 10^{10} G dipolar magnetic field, as a model of a neutron-star-powered ultraluminous X-ray source (ULX). We compute a lower limit on the total luminosity of 2.5LEdd\sim 2.5\,L_\mathrm{Edd}, and find the radiation... Show more
July 2, 2021
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Beamed emission from a neutron-star ULX in a GRRMHD simulation
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