2019
DOI: 10.1103/physrevc.100.035205
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Chiral light-front perturbation theory and the flavor dependence of the light-quark nucleon sea

Abstract: The light-quark flavor dependence of the proton sea has been of great interest for many years because of its close connection with non-perturbative effects. One hypothesis is that this dependence arises from the pion cloud of the proton. We apply light cone perturbation theory and experimental constraints to a chiral Lagrangian to compute the relevant Fock-space components of the nucleon wave function with well-defined uncertainties. Existing experimental information regarding the light flavor sea is studied, … Show more

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Cited by 20 publications
(12 citation statements)
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“…The correlations of the statistical uncertainties of σD/(2σH) were propagated through the d/ū extraction. The dependence on the value for the 26 and the green band shows the predictions of the statistical parton distributions of Basso, Bourrely, Pasechnik and Soffer 22 . The red solid (blue dashed) curves show the calculated ratios of d(x) to ū(x) with CT18 30 (CTEQ6 36 ) parton distributions at the scales of the SeaQuest results.…”
mentioning
confidence: 59%
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“…The correlations of the statistical uncertainties of σD/(2σH) were propagated through the d/ū extraction. The dependence on the value for the 26 and the green band shows the predictions of the statistical parton distributions of Basso, Bourrely, Pasechnik and Soffer 22 . The red solid (blue dashed) curves show the calculated ratios of d(x) to ū(x) with CT18 30 (CTEQ6 36 ) parton distributions at the scales of the SeaQuest results.…”
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confidence: 59%
“…21,22 Another class including chiral soliton models 23 and meson-baryon models emphasize mesonic degrees of freedom in proton structure. [24][25][26] These latter models (statistical, chiral soliton, and meson-baryon) each attempt to describe the entire non-perturbative composition of the proton. A common feature of these models is a rise in the d/ū flavor asymmetry with x.…”
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confidence: 99%
“…A recent (October 2017) Institute for Nuclear Theory Workshop, "The Flavor Structure of the Nucleon Sea", provides an excellent overview Figure 11. The upper graph shows the NUSEA [12]d/ū data compared to the hadron model calculation of Alberg and Miller [74] and the statistical parton distribution fit of Bourrely and Soffer [32]. The lower plot showsd −ū from NUSEA [12] and HERMES [15] along with an instanton model [75], chiral quark solition model [34], the meson cloud model of Alberg and Miller [74] and the statistical parton distribution fit [32].…”
Section: Calculations and Models Of The Sea Distributionsmentioning
confidence: 99%
“…Many of these issues have been handled by Alberg and Miller [103]. Recent predictions of the Alberg and Miller calculations in the context of chiral light front perturbation theory [74] are shown in Fig. 11.…”
Section: Hadron Modelsmentioning
confidence: 99%
“…xxi 2.24d(x)/ū(x) prediction (grey band) for the meson cloud model [61]. Blue points are E866 data points.…”
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confidence: 99%