Nearly universal inverse mappings between neutron star radius R1.4 and empirical EOS parameters cause precision-dependent shifts in Bayesian posterior means via nonlinear filtering of the radius distribution.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
nucl-th 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Trace anomaly of cold dense matter extracted from heavy-ion flow observables matches neutron-star posterior bands, establishing a composition-insensitive bridge between the two environments.
citing papers explorer
-
Universal EOS-Radius Inverse Mappings Govern Precision-Dependent Inference of the Neutron Star Equation of State
Nearly universal inverse mappings between neutron star radius R1.4 and empirical EOS parameters cause precision-dependent shifts in Bayesian posterior means via nonlinear filtering of the radius distribution.
-
Trace Anomaly of Cold Dense Matter Constrained by Collective Flow
Trace anomaly of cold dense matter extracted from heavy-ion flow observables matches neutron-star posterior bands, establishing a composition-insensitive bridge between the two environments.