Regge trajectory relations for the universal description of the heavy-light systems: diquarks, mesons, baryons and tetraquarks
Abstract
Two newly proposed Regge trajectory relations are employed to analyze the heavy-light systems. One of the relations is M=m1+m2+C'+βxx+c0x, (x=l,\,nr). Another reads M=m1+C'+βx2(x+c0x)+43πβxm3/22(x+c0x)1/4. M is the bound state mass. m1 and m2 are the masses of the heavy constituent and the light constituent, respectively. l is the orbital angular momentum and nr is the radial quantum number. βx and c0x are fitted. m1, m2 and C' are input parameters. These two formulas consider both of the masses of heavy constituent and light constituent. We find that the heavy-light diquarks, the heavy-light mesons, the heavy-light baryons and the heavy-light tetraquarks satisfy these two formulas. When applying the first formula, the heavy-light systems satisfy the universal description irrespective of both of the masses of the light constituents and the heavy constituent. When using the second relation, the heavy-light systems satisfy the universal description irrespective of the mass of the heavy constituent. The fitted slopes differ distinctively for the heavy-light mesons, baryons and tetraquarks, respectively. When employing the first relation, the average values of cfnr (cfl) are 1.026, 0.794 and 0.553 (1.026, 0.749 and 0.579) for the heavy-light mesons, the heavy-light baryons and the heavy-light tetraquarks, respectively. Upon application of the second relation, the mean values of cfnr (cfl) are 1.108, 0.896 and 0.647 (1.114, 0.855 and 0.676) for the heavy-light mesons, the heavy-light baryons and the heavy-light tetraquarks, respectively. Moreover, the fitted results show that the Regge trajectories for the heavy-light systems are concave downwards in the (M2,\,nr) and (M2,\,l) planes.
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