2009
DOI: 10.1186/1754-0410-3-1
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Weinberg like sum rules revisited

Abstract: The generalized Weinberg sum rules containing the difference of isovector vector and axial-vector spectral functions saturated by both finite and infinite number of narrow resonances are considered. We give a historical survey and summarize the status of these sum rules analyzing their overall agreement with phenomenological Lagrangians, lowenergy relations, parity doubling, hadron string models, and experimental data.

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Cited by 10 publications
(7 citation statements)
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References 114 publications
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“…The simplest SW holographic models can be viewed as the most selfconsistent way of rewriting the infinite number of pole terms (expected in the large-N c limit of QCD [47,48]) with linear spectrum of masses squared, in the pole representation of two-point Correlation Functions (CFs), as some 5D gravitational model of free fields [49,50]. This means, in particular, that the SW holographic models are closely related with the planar QCD sum rules which were widely used in the past to study the phenomenology of linear radial trajectories in the meson sector [51]. In the field of deep inelastic scattering, the holographic approach, especially the SW one, recovers the old pre-QCD dual description with all its phenomenological successes [17].…”
Section: Introductionmentioning
confidence: 99%
“…The simplest SW holographic models can be viewed as the most selfconsistent way of rewriting the infinite number of pole terms (expected in the large-N c limit of QCD [47,48]) with linear spectrum of masses squared, in the pole representation of two-point Correlation Functions (CFs), as some 5D gravitational model of free fields [49,50]. This means, in particular, that the SW holographic models are closely related with the planar QCD sum rules which were widely used in the past to study the phenomenology of linear radial trajectories in the meson sector [51]. In the field of deep inelastic scattering, the holographic approach, especially the SW one, recovers the old pre-QCD dual description with all its phenomenological successes [17].…”
Section: Introductionmentioning
confidence: 99%
“…[2,3] for calculation of CFs follows in a natural way within such a rewriting. This means, in particular, that the SW holographic models are closely related with the planar QCD sum rules (in a sense, they represent just 5D rewriting of those sum rules [68]) which were widely used in the past to study the phenomenology of linear radial trajectories in the meson sector [70]. In descriptions of hadron electromagnetic form factors, the holographic approach, especially the SW one, recovers the old pre-QCD dual description with all its phenomenological successes [27].…”
Section: Introductionmentioning
confidence: 99%
“…We checked also other variants with inputs corresponding to f π = 87 MeV in Table 1 and with α s = 0 in (28). They result in a shift within 70-80 MeV for masses that lies within the accuracy of the large-N c limit.…”
Section: Scalar Sum Rulesmentioning
confidence: 99%
“…The quantities M σ , G σ , G = g (where g is defined in (29)), and mass of the first state on the scalar trajectory are plotted in Fig. 2 using the inputs from Table 1 for f π = 93 MeV and α s 1/π in (28) that was obtained in the vector case. The intercept m 2 s can be negative as the sum in (23) begins with n = 1.…”
Section: Scalar Sum Rulesmentioning
confidence: 99%
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