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.
This is the case for nucleon-nucleon bremsstrahlung (j), as the kernel depends on the sum of neutrino energies
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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.