Preprint
Oct 2026
Adiabatic evolution of hadronic neutron stars
In this paper we compute several structural properties of static and rotating neutron stars, considering both rigid and differential rotation. To this end, we use a finite-temperature beta-stable equation of state (EOS) extending the zero-temperature hadronic EOS derived by Fortin et al. (2017). We account for the form...
D. Logoteta, Francesco Zeno Constanzo, I. Bombaci et al.
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