Abstract

By applying the Bohr–Sommerfeld quantization approach to the quadratic form of the spinless Salpeter-type equation (QSSE), we show that the obtained Regge trajectories for the mesons consisting of unequally massive quarks take the form M^2=beta left( {c_l}l+{pi }n_r+c_0right) ^{2/3}+c_1, which have the same form as the Regge trajectories for charmonia and bottomonia. Then we apply the obtained Regge trajectories to fit the spectra of the strange mesons, the heavy-light mesons (the D, D_s, B and B_s mesons) and the bottom-charmed mesons. The fitted Regge trajectories are in agreement with the experimental data and the theoretical predictions, which demonstrates that the newly proposed Regge trajectories can be applied universally to the light mesons, the heavy-light mesons and the heavy mesons. By fitting the spectra of the mesons composed of different quarks, the concavity of these Regge trajectories are illustrated, which is of cardinal significance for the potential models.

Highlights

  • We use the quadratic form of the spinless Salpeter-type equation (QSSE) [26,27,28,29,30,31,32,33] to discuss the Regge trajectories for the mesons consisting of different quarks

  • We notice that the Regge trajectories for these meson are concave, which is of cardinal significance for the potential models because this property of the Regge trajectories can assist in the choice of the appropriate dynamic equation and potential to describe mesons

  • In Ref. [25], we have shown that the bottomonia and charmonia can be well described by the concave formula (1)

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Summary

Introduction

The Regge trajectory is one of the effective approaches for studying hadron spectra [1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22]. We use the quadratic form of the spinless Salpeter-type equation (QSSE) [26,27,28,29,30,31,32,33] to discuss the Regge trajectories for the mesons consisting of different quarks. 2, the new form of the Regge trajectories for mesons composed of different quarks is obtained from the QSSE, which has the same form as that for heavy quarkonia. 3, the obtained Regge trajectory is applied to fit the spectra of the strange mesons, the heavy-light mesons and the bottom-charmed mesons. 4, the universality and concavity of the newly proposed Regge trajectories are discussed.

Regge trajectories from the QSSE
Regge trajectories for the mesons composed of different quarks
Regge trajectories for the mesons constituting of different quarks
Strange mesons
Charmed mesons
Charmed-strange mesons
12 LNR KDR
Universality of the new form of the Regge trajectories
Concavity of the Regge trajectories
Conclusions
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