Fractionized Skyrmions in Dense Compact-Star Matter
Masayasu Harada, Hyun Kyu Lee, Yong-Liang Ma, Mannque Rho

TL;DR
This paper explores a novel phase of dense hadronic matter where skyrmions fractionize into half-skyrmions, leading to a phase with restored chiral symmetry but confined quarks, impacting the equation of state in neutron stars.
Contribution
It introduces the concept of a half-skyrmion phase in dense matter, characterized by specific symmetry properties and its role in the transition of the equation of state in compact stars.
Findings
Identification of a half-skyrmion phase at density n_{1/2}
Chiral symmetry is globally restored with confined quarks
Implication for a stiffer equation of state in neutron stars
Abstract
The hadronic matter described as a skyrmion matter embedded in an FCC crystal is found to turn into a half-skyrmion matter with vanishing (in the chiral limit) quark condensate and {\it non-vanishing} pion decay constant {} at a density lower than or near the critical density at which hadronic matter changes over to a chiral symmetry restored phase with possibly deconfined quarks. When hidden local gauge fields and a dilaton scalar of spontaneously broken scale symmetry with decay constant are incorporated, this half-skyrmion phase is characterized by with the hidden gauge coupling but . While chiral symmetry is restored {\it globally} in this region in the sense that space-averaged, vanishes, quarks are still confined in massive hadrons and massless pions. This phase is shown to play a crucial…
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