Binary neutron star merger simulations with consistent muon treatment show ejecta masses reduced by at most 17% while average electron fractions, velocities, and temperatures differ by less than 6% from non-muonic cases.
(C23)-(C24), to be evaluated at fixedY µ
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Consistent Treatment of Muons in Binary Neutron Star Mergers
Binary neutron star merger simulations with consistent muon treatment show ejecta masses reduced by at most 17% while average electron fractions, velocities, and temperatures differ by less than 6% from non-muonic cases.