$\Delta$-admixed neutron stars: spinodal instabilities and dUrca processes

TL;DR

This paper models $$-admixed neutron stars using covariant density functional theory, revealing phase transitions affecting star properties and conditions for direct Urca processes within astrophysical constraints.

Contribution

It introduces a comprehensive equation of state for $$-admixed stars considering uncertainties in $(1232)$ interactions, highlighting phase transitions and their astrophysical implications.

Findings

First order phase transition in $$-admixed matter persists at finite temperature.

Compact stars with such phase transitions have small radii and tidal deformabilities.

Parameter space allows for maximum mass constraints and direct Urca processes.

Abstract

Within the covariant density functional theory of nuclear matter we build equations of state of $\Delta$-admixed compact stars. Uncertainties in the interaction of $\Delta(1232)$ resonance states with nuclear matter, due to lack of experimental data, are accounted for by varying the coupling constants to scalar and vector mesonic fields. We find that, over a wide range of the parameter space allowed by nuclear physics experiments and astrophysical observations, cold catalyzed star matter exhibits a first order phase transition which persists also at finite temperature and out of $\beta$-equilibrium in the neutrino-transparent matter. Compact stars featuring such a phase transition in the outer core have small radii and, implicitly, tidal deformabilities. The parameter space is identified where simultaneously $\Delta$-admixed compact stars obey the astrophysical constraint on maximum mass and allow for dUrca processes, which is otherwise forbidden.