Twins in the Shadow: Phase Transitions in Proto-Neutron Stars
astro-ph.HE, nucl-th
Submitted: 2026-10-02
Updated: 2026-10-02
Terminology
Sources
- Core-Collapse Supernova Explosion Theory
- Hydrodynamics of core-collapse supernovae and their progenitors
- Evolution of Protoneutron Stars
- Proto-Neutron and Neutron Stars in a Chiral SU(3) Model
- Hybrid stars that masquerade as neutron stars
- Investigation of the existence of hybrid stars using Nambu-Jona-Lasinio models
- Hybrid stars with the Dyson-Schwinger quark model
- Hadron-Quark Crossover and Massive Hybrid Stars with Strangeness
- Finite-size effects at the hadron-quark transition and heavy hybrid stars
- Stable hybrid stars within a SU(3) Quark-Meson-Model
- Bayesian inference of dense matter EOS encapsulating a first-order hadron-quark phase transition from observables of canonical neutron stars
- Maximum mass of neutron stars and strange neutron-star cores
- High-mass twins & resolution of the reconfinement, masquerade and hyperon puzzles of compact star interiors
- Twin Stars within the SU(3) Chiral Quark-Meson Model
- Signals in the tidal deformability for phase transitions in compact stars with constraints from GW170817
- Astrophysical aspects of general relativistic mass twin stars
- Neutron Star Equation of State in light of GW190814
- Generic conditions for stable hybrid stars
- Constraining and applying a generic high-density equation of state
- Compact stars with sequential QCD phase transitions
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