Existence of a hadron–quark phase transition in neutron star cores
Determine whether dense matter in the cores of neutron stars undergoes a phase transition from hadronic matter to deconfined quark matter.
References
It remains an open question of whether the phase transition (PT) from hadronic to quark matter occurs in the cores of NSs - the densest matter found in the Universe.
— First-order phase transitions in the cores of neutron stars
(2404.05637 - Komoltsev, 2024) in Introduction (Section 1)
This overlap leads us to conjecture that it may correspond to a region in which nucleonic and quark degrees of freedom coexist.
— Thermodynamic signatures do not uniquely identify deconfinement in neutron stars
(2610.01701 - Ma et al., 1 Oct 2026) in Main text, paragraph comparing nucleonic, quark-matter, and quarkyonic equations of state
Therefore, the structural characteristics of neutron stars composed of cold and dense matter, as well as whether a hadron-quark phase transition exists in their cores, remain an open question.
— Axion effects on hybrid stars: earlier hadron-quark phase transition and larger quark-matter cores
(2610.09480 - Liu et al., 7 Oct 2026) in Section I, Introduction