Bayesian analysis of NICER and small-radius pulsar data favors a strong first-order phase transition at 2.7-2.8 nuclear densities with a 600-700 MeV energy jump and high post-transition sound speed, producing twin stars of 6-7 km radius and strongly suppressed tidal deformability.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
The quark-hadron mixed phase width in hybrid stars is mainly controlled by effective nucleon mass and symmetry energy, with temperature reducing the width and softening the EOS while strong vector repulsion is needed to match massive pulsar and NICER data.
citing papers explorer
-
Bayesian Inference of Dense-Matter Equations of State from Small-Radius Compact Stars with Twin-Star Scenarios
Bayesian analysis of NICER and small-radius pulsar data favors a strong first-order phase transition at 2.7-2.8 nuclear densities with a 600-700 MeV energy jump and high post-transition sound speed, producing twin stars of 6-7 km radius and strongly suppressed tidal deformability.
-
Characterizing the quark-hadron mixed phase in compact star cores : sensitivity to nuclear saturation and quark-model parameters at finite-temperature
The quark-hadron mixed phase width in hybrid stars is mainly controlled by effective nucleon mass and symmetry energy, with temperature reducing the width and softening the EOS while strong vector repulsion is needed to match massive pulsar and NICER data.