Skyrmions with vector mesons in the hidden local symmetry approach

preprint2013arXivOpen access

Abstract

The roles of light ρρ and ωω vector mesons in the Skyrmion are investigated in a chiral Lagrangian derived from the hidden local symmetry (HLS) up to O(p4)O(p^4) including the homogeneous Wess-Zumino (hWZ) terms. We write a general "master formula" that allows us to determine the parameters of the HLS Lagrangian from a class of holographic QCD models valid at large NcN_c and λλ ('t Hooft constant) limit by integrating out the infinite towers of vector and axial-vector mesons other than the lowest ρρ and ωω mesons. Within this approach we find that the physical properties of the Skyrmion as the solitonic description of baryons are \textit{independent} of the HLS parameter aa. Therefore the only parameters of the model are the pion decay constant and the vector meson mass. Once determined in the meson sector, we have a totally parameter-free theory that allows us to study unequivocally the role of light vector mesons in the Skyrmion structure. We find, as suggested by Sutcliffe, that inclusion of the ρρ meson reduces the soliton mass, which makes the Skyrmion come closer to the Bogomol'nyi-Prasad-Sommerfield (BPS) soliton, but the role of the ωω meson is found to increase the soliton mass. In a stark contrast, the ΔΔ-NN mass difference, which is determined by the moment of inertia in adiabatic collective quantization of the Skyrmion, is increased by the ρρ vector meson, while it is reduced by the inclusion of the ωω meson. All these observations show the importance of the ωω meson in the properties of the nucleon and nuclear matter in the Skyrme model.

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