A constrained Gaussian-process bridge prior generates model-agnostic, nonparametric, thermodynamically consistent priors for neutron-star equation-of-state inference.
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Requiring causal stable thermodynamically consistent extensions of neutron-star EOS models to perturbative QCD constrains high-density behavior and disfavors purely nucleonic descriptions for all stable stars.
Tripling fluctuations in a BEC-BCS-inspired model provide a microscopic derivation of quarkyonic matter that reproduces the speed of sound peak and baryon momentum shell in a simplified dense-matter framework.
Hierarchical Bayesian and ML analysis of magnetar observables finds no statistically significant need for a distinct white-dwarf magnetar population.
citing papers explorer
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Constrained Gaussian-process bridge prior for neutron-star equation-of-state inference
A constrained Gaussian-process bridge prior generates model-agnostic, nonparametric, thermodynamically consistent priors for neutron-star equation-of-state inference.
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As above, so below: assessing extremeness of the neutron-star equation of state based on the unstable branch
Requiring causal stable thermodynamically consistent extensions of neutron-star EOS models to perturbative QCD constrains high-density behavior and disfavors purely nucleonic descriptions for all stable stars.
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Quarkyonic matter and hadron-quark crossover from an ultracold atom perspective
Tripling fluctuations in a BEC-BCS-inspired model provide a microscopic derivation of quarkyonic matter that reproduces the speed of sound peak and baryon momentum shell in a simplified dense-matter framework.
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Data-Driven Constraints on Magnetar Population: No Evidence for a Distinct White Dwarf Channel
Hierarchical Bayesian and ML analysis of magnetar observables finds no statistically significant need for a distinct white-dwarf magnetar population.