In the most elementary description of ground-state baryons, one would simply add the effective constituent masses, i.e., the masses would depend linearly upon the flavour numbers. Now, if one introduces a central, flavour–independent potential and solves accurately the three-body problem, one should hope to get something appreciably different. To measure to what extent this is true, let us define the scale-independent quantities
![]() | (11.2) |
![]() | (11.3) |
R1 is relevant for possible deviations from the Gell-Mann–Okubo mass formula, R1 and R2 for the equal spacing rule of the decuplet. R1 and R2 are expected to be negative, as shown in Section 8.2. The effect is of the order of 5–10% in magnitude for typical choices ms < ∼ mq, as seen in Fig. 11.1, where various power-law potentials rβ and quark mass ratios m s∕mq are used. The ratios R1 and R2 were already displayed in Ref. [58] in a slightly different way. It is shown, in particular, that one hardly differentiates a three-body Y-shape potential (see Eq. 9.14) from a genuinely additive linear potential.
In Fig. 11.2, we show the variations of the binding energy of qqQ as a function of the inverse of the mass mQ of the heavy quark. The energy qqQ is almost linear in mQ−1, as conjectured in Ref. [87].