On accretion discs formed in MHD simulations of black hole–neutron star mergers with accurate microphysics
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DOI: 10.1093/mnras/stab1824
Abstract: Remnant accretion discs formed in compact object mergers are an important ingredient in the understanding of electromagnetic afterglows of multimessenger gravitational-wave events. Due to magnetically and neutrino-driven winds, a significant fraction of the disc mass… read more here.
Keywords: discs formed; hole neutron; accretion discs; black hole ... See more keywords