2013
DOI: 10.1103/physrevc.87.054332
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Half-Skyrmions and the equation of state for compact-star matter

Abstract: The half-skyrmions that appear in dense baryonic matter when skyrmions are put on crystals modify drastically hadron properties in dense medium and affect strongly the nuclear tensor forces, thereby influencing the equation of state (EoS) of dense nuclear and asymmetric nuclear matter. The matter comprised of half skyrmions has vanishing quark condensate but non-vanishing pion decay constant and could be interpreted as a hadronic dual of strong-coupled quark matter. We infer from this observation combined with… Show more

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Cited by 35 publications
(94 citation statements)
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“…Recently, the study of parity doublet structure using lattice QCD [33] shows that the positive parity nucleon mass changes very small near the deconfinement transition, which may imply that m 0 does exist in nature and its value is close to the positive parity nucleon mass. The existence of chiral invariant mass is also discussed in the context of Skyrmion crystal [34].…”
Section: Phase Diagrammentioning
confidence: 99%
“…Recently, the study of parity doublet structure using lattice QCD [33] shows that the positive parity nucleon mass changes very small near the deconfinement transition, which may imply that m 0 does exist in nature and its value is close to the positive parity nucleon mass. The existence of chiral invariant mass is also discussed in the context of Skyrmion crystal [34].…”
Section: Phase Diagrammentioning
confidence: 99%
“…Now a comment on the role of a non-zero chiral invariant mass m 0 in nuclear physics. When nuclear matter is described in effective field theory anchored on the low-momentum nuclear interaction V low−k derived via Wilsonian renormalization group equations, how the nucleon mass scales in medium as a function of density turns out to be quite important for the structure of finite nuclei as well as nuclear matter [28,29]. The presence of a substantially big m 0 as is found in some analysis in medium [22] would affect crucially how the nucleon mass scales in density in such effective field theory approach to nuclei, nuclear matter and dense compact-star matter.…”
Section: Remarks and Conclusionmentioning
confidence: 99%
“…Though not firm, this feature is not inconsistent with what is observed with the EoS of compact-star matter [22]. This means that the ω meson-exchange contribution to the Weinberg-Tomozawa term in medium will be the same as the local form in the vacuum.…”
Section: Hidden Local Symmetry With Scale Invariancementioning
confidence: 51%
“…As in Appendix A, we refer to (22) as "case 1" and (23) as "case 2". From (21), we get for the two cases of possible scaling:…”
Section: Scalingmentioning
confidence: 99%