English

Light-meson orbital excitations in the QCD string approach

High Energy Physics - Phenomenology 2009-11-07 v2 High Energy Physics - Experiment

Abstract

In the framework of the QCD string approach it is shown that the spin-averaged masses Mˉ(nL)\bar{M}(nL) of all low-lying light mesons are well described using the string tension σ\sigma as the only parameter. The Regge slope αL\alpha'_L and the intercept αL(0)\alpha_L(0) of the Regge L-trajectory for Mˉ(nL)\bar{M}(nL) are calculated analytically and turn out to be αL=0.80\alpha'_L = 0.80 GeV2{}^{-2} (for L4L \leq 4) and αL(0)=0.34\alpha_L(0) = -0.34, in good agreement with the experimental data: αLexp=0.81±0.01\alpha'_{L {\rm exp}} = 0.81 \pm 0.01 GeV2{}^{-2}, αLexp(0)=0.30±0.02\alpha_{L {\rm exp}}(0) = -0.30 \pm 0.02. To obtain this strong agreement with the data the nonperturbative quark self-energy contributions to the meson masses must be taken into account, which appeared to be large and negative for small values of L, and are even for larger values of L important for a close fit. From the present analysis of the meson spectra the restriction αs0.40\alpha_s \leq 0.40 on the strong coupling is required.

Keywords

Cite

@article{arxiv.hep-ph/0202246,
  title  = {Light-meson orbital excitations in the QCD string approach},
  author = {A. M. Badalian and B. L. G. Bakker},
  journal= {arXiv preprint arXiv:hep-ph/0202246},
  year   = {2009}
}

Comments

18 pages RevTeX, 1 figure

R2 v1 2026-07-22T13:39:35.004Z