Bayesian analysis of causal hybrid EOS models constrained by neutron-star observations favors a maximum mass of 2.2-2.3 solar masses with radius near 12 km, largely independent of the hadronic baseline.
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Maximal mass of neutron stars constrained by neutron star observations
Bayesian analysis of causal hybrid EOS models constrained by neutron-star observations favors a maximum mass of 2.2-2.3 solar masses with radius near 12 km, largely independent of the hadronic baseline.