SU(3) parity doubling in cold neutron star matter

Fraga, Eduardo S.; da Mata, Rodrigo; Schaffner-Bielich, Jürgen

doi:10.1103/physrevd.108.116003

Phys. Rev. D

2023

DOI: 10.1103/physrevd.108.116003

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SU(3) parity doubling in cold neutron star matter

Eduardo S. Fraga,

Rodrigo da Mata,

Jürgen Schaffner-Bielich

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2024

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Cited by 4 publications

References 79 publications

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Thermodynamics of the parity-doublet model: Symmetric nuclear matter and the chiral transition

Eser,

Blaizot

2024

Phys. Rev. C

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Thermodynamics of the parity-doublet model: Symmetric nuclear matter and the chiral transition

Eser,

Blaizot

2024

Phys. Rev. C

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Which first order phase transitions to quark matter are possible in neutron stars?

Christian,

Schaffner-Bielich,

Rosswog

2024

Phys. Rev. D

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Anatomy of critical fluctuations in hadronic matter

Marczenko

2024

Phys. Rev. D

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Critical phenomena in phase transitions of strongly interacting matter, governed by quantum chromodynamics, are inherently encoded in the fluctuations of conserved charges. In this work, we study the net-baryon number density fluctuations, including the lowest-lying nucleon and the baryonic resonance Δ(1232), based on the parity doublet model in the mean-field approximation. We focus on the qualitative features of the second-order susceptibility of the net-baryon number density in dense hadronic matter and how the inclusion of Δ(1232) affects it. We demonstrate that the fluctuations of the individual baryons do not necessarily reflect the total net-baryon number fluctuations at finite density, due to the nontrivial correlations between different particle species. Our results highlight the role of baryonic correlations in the interpretation of data from heavy ion collision experiments. Published by the American Physical Society 2024

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SU(3) parity doubling in cold neutron star matter

Cited by 4 publications

References 79 publications

Thermodynamics of the parity-doublet model: Symmetric nuclear matter and the chiral transition

Thermodynamics of the parity-doublet model: Symmetric nuclear matter and the chiral transition

Which first order phase transitions to quark matter are possible in neutron stars?

Anatomy of critical fluctuations in hadronic matter

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