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.
Prospect of unraveling the first-order phase transition in neutron stars with f and p _ 1 modes
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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.