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Asymptotically causal metamodel for neutron star equations of state
Phys. Rev. D 114, 103022 – Published 10 November, 2026
DOI: https://doi.org/10.1103/bv9r-hvhm
Abstract
Nuclear metamodels—phenomenological parametrizations of the energy of nuclear matter—are convenient tools to explore the space of realistic neutron star configurations constrained by astrophysical and nuclear data. While much recent work has focused on composition-agnostic barotropic models, the metamodel approach is designed to describe the composition dependence of the relevant thermodynamic potential. We revise a previously proposed nonrelativistic metamodel by introducing a more controlled high-density behavior, improving both its causal properties and its accuracy in reproducing the pressure and the -equilibrium composition of microscopically motivated equations of state. Since asymptotic causality is enforced by construction, the fraction of discarded models due to superluminal sound speeds is substantially reduced, facilitating metamodel-based explorations of equilibrium neutron star configurations. We further assess our framework by performing a Bayesian inference of neutron star properties beyond standard observables such as masses and radii, exploiting the metamodel’s ability to probe composition-dependent quantities including the dUrca threshold and the Ledoux criterion for g-mode stability.
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