Bayesian analysis of NICER+GW170817 data over three agnostic EoS ensembles suggests observations favor a soft-to-stiff EoS shape resembling the maximum-compactness sequence, not the maximum-mass sequence.
Combustion adiabat and the maximum mass of a quark star
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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars?
Bayesian analysis of NICER+GW170817 data over three agnostic EoS ensembles suggests observations favor a soft-to-stiff EoS shape resembling the maximum-compactness sequence, not the maximum-mass sequence.