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Non-Abelian chiral soliton lattice in rotating QCD matter: Nambu-Goldstone and excited modes
Non-Abelian chiral soliton lattice in rotating QCD matter: Nambu-Goldstone and excited modes
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Non-Abelian chiral soliton lattice in rotating QCD matter: Nambu-Goldstone and excited modes
Non-Abelian chiral soliton lattice in rotating QCD matter: Nambu-Goldstone and excited modes

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Non-Abelian chiral soliton lattice in rotating QCD matter: Nambu-Goldstone and excited modes
Non-Abelian chiral soliton lattice in rotating QCD matter: Nambu-Goldstone and excited modes
Journal Article

Non-Abelian chiral soliton lattice in rotating QCD matter: Nambu-Goldstone and excited modes

2024
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Overview
A bstract The ground state of QCD with two flavors at a finite baryon chemical potential under rapid rotation is a chiral soliton lattice (CSL) of the η meson, consisting of a stack of sine-Gordon solitons carrying a baryon number, due to the anomalous coupling of the η meson to the rotation. In a large parameter region, the ground state becomes a non-Abelian CSL, in which due to the neutral pion condensation each η soliton decays into a pair of non-Abelian sine-Gordon solitons carrying S 2 moduli originated from Nambu-Goldstone (NG) modes localized around it, corresponding to the spontaneously broken vector symmetry SU(2) V . There, the S 2 modes of neighboring solitons are anti-aligned, and these modes should propagate in the transverse direction of the lattice due to the interaction between the S 2 modes of neighboring solitons. In this paper, we calculate excitations including gapless NG modes and excited modes around non-Abelian and Abelian ( η ) CSLs, and find three gapless NG modes with linear dispersion relations (type-A NG modes): two isospinons ( S 2 modes) and a phonon corresponding to the spontaneously broken vector SU(2) V and translational symmetries around the non-Abelian CSL, respectively, and only a phonon for the Abelian CSL because of the recovering SU(2) V . We also find in the deconfined phase that the dispersion relation of the isospinons becomes of the Dirac type, i.e. linear even at large momentum.