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arXiv · 2603.16019

Sensitivity of neutron star observables to microscopic nuclear parameters of realistic equations of state

Nikolas Cruz-Camacho·Carlos Conde-Ocazionez·Veronica Dexheimer·Jacquelyn Noronha-Hostler·Nicolás Yunes
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Abstract

The equation of state of matter at supranuclear densities governs the astrophysical observables of neutron stars. A realistic, though complex, description is provided by the Chiral-Mean-Field model, which depends on many microscopic nuclear-physics parameters. We present a Fisher-information-inspired analysis of the sensitivity of neutron-star observables to the parameters of the Chiral-Mean-Field model at $\beta$-equilibrium using SLy as a crust. We then compute neutron-star sequences and extract masses, radii, compactnesses, and tidal deformabilities. From the logarithmic derivatives of these observables with respect to each nuclear parameter, we construct a dimensionless, Fisher-inspired sensitivity matrix and perform a principal-component analysis to identify the effective combinations of nuclear parameters that most strongly affect neutron-star observables. Although the ranking depends mildly on the observable, the three most important nuclear parameters are the vacuum value of the dilaton field $\chi_0$ (which sets the overall scale of the scalar potential and trace-anomaly contribution), the scalar singlet strength $g_{1}^X$ (which controls the overall scalar attraction through the baryon effective masses), and the $k_0$ quadratic scalar term (which governs the curvature of the scalar potential). This framework provides a reproducible, data-driven approach to quantify parameter sensitivities in dense-matter models and to guide future Bayesian inference of nuclear information from multi-messenger astrophysical observations.

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Nikolas Cruz-Camacho, Carlos Conde-Ocazionez, Veronica Dexheimer, Jacquelyn Noronha-Hostler, Nicolás Yunes. 2026-03-16. Sensitivity of neutron star observables to microscopic nuclear parameters of realistic equations of state. https://arxiv.org/abs/2603.16019

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