Some aspects of the phase diagram of nuclear matter relevant to compact stars
F. Gulminelli (LPCC), Ad-R. Raduta, J. Margueron (IPNO), P., Papakonstantinou (IPNO), M. Oertel

TL;DR
This paper explores phase transitions in dense nuclear matter relevant to neutron stars and supernovae, focusing on the crust-core transition and hyperonic effects, with implications for the matter's equation of state and astrophysical phenomena.
Contribution
It introduces a quasi-particle model for the crust-core transition and analyzes hyperonic phase transitions using a mean-field approach, highlighting new insights into dense matter behavior.
Findings
Clusterized phase due to Coulomb interactions not accessible in grand-canonical ensemble
Quantitative results for supernova dynamics from the quasi-particle model
Characteristics and order of hyperonic phase transitions analyzed
Abstract
Dense matter as it can be found in core-collapse supernovae and neutron stars is expected to exhibit different phase transitions which impact the matter composition and the equation of state, with important consequences on the dynamics of core-collapse supernova explosion and on the structure of neutron stars. In this paper we will address the specific phenomenology of two of such transitions, namely the crust-core solid-liquid transition at sub-saturation density, and the possible strange transition at super-saturation density in the presence of hyperonic degrees of freedom. Concerning the neutron star crust-core phase transition at zero and finite temperature, it will be shown that, as a consequence of the presence of long-range Coulomb interactions, a clusterized phase is expected which is not accessible in the grand-canonical ensemble. A specific quasi-particle model will be…
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