2002
DOI: 10.1016/s0375-9474(01)01670-0
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Solitons in nonlocal chiral quark models

Abstract: Properties of hedgehog solitons in a chiral quark model with nonlocal regulators are described. We discuss the formation of the hedgehog soliton, the quantization of the baryon number, the energetic stability, the gauging and construction of Noether currents with help of path-ordered P-exponents, and the evaluation of observables. The issue of nonlocality is thoroughly discussed, with a focus on contributions to observables related to the Noether currents. It is shown that with typical model parameters the sol… Show more

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Cited by 41 publications
(35 citation statements)
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“…The non-local character of the interactions arises naturally in the context of several successful approaches to low-energy quark dynamics, and leads to a momentum dependence in the quark propagator that can be made consistent [16] with lattice results. It has been shown [17][18][19][20] that non-local models …”
mentioning
confidence: 99%
“…The non-local character of the interactions arises naturally in the context of several successful approaches to low-energy quark dynamics, and leads to a momentum dependence in the quark propagator that can be made consistent [16] with lattice results. It has been shown [17][18][19][20] that non-local models …”
mentioning
confidence: 99%
“…On the other hand, the inclusion of meson self-interaction which allows for a substantial deviation of the σ-field from its vacuum value inside the baryon considerably increases C A 5 . The LSM overestimates this contribution, but this is not the case in other chiral models which allow for a non-zero fluctuation of the σ-field; in a version of the NJL model with nonlocal regulators [13] the contribution of sea quarks to the nucleon g A is more than a factor of two weaker than the equivalent contribution of chiral mesons in the LSM.…”
Section: Resultsmentioning
confidence: 90%
“…For fixed values of the temperature T and the chemical potential µ, the mean field valuesσ and∆, as well as the chemical potentials µ e and µ 8 , can be numerically obtained from the gap equations (13), together with the neutron star constraints (18) and (19). Let us begin by considering the case H/G = 0.75, which is motivated by various effective models of quark-quark interactions.…”
Section: B Order Parameters and Phase Transitionsmentioning
confidence: 99%
“…Indeed, nonlocal interactions regularize the models in such a way that anomalies are preserved [13] and charges properly quantized, the effective interaction is finite to all orders in the loop expansion and there is no need to introduce extra cut-offs, soft regulators lead to small nextto-leading order corrections [14], etc. This type of models has been successfully used to investigate meson [15][16][17][18] and baryon [19] properties at vanishing temperature and chemical potential, and the phase diagram of isospin symmetric matter has also been studied within this context [20][21][22][23]. Now our aim is to extend these analyses to the case in which compact star conditions are imposed.…”
Section: Introductionmentioning
confidence: 99%