Low-lying spectrum of the Y-string three-quark potential using hyper-spherical coordinates

TL;DR

This paper calculates the energies of three-quark states under the Y-string potential using hyper-spherical coordinates, improving approximation methods to understand the spectrum and energy splittings with high precision.

Contribution

It introduces a multi-level approximation approach to accurately compute three-quark energies with the Y-string potential, including exact minimal-length string considerations.

Findings

Exact non-perturbative corrections are about 1% of total energy.

Energy differences between multiplets follow a 2:2:0.9 ratio, deviating from the 2:2:1 rule.

The Roper resonance remains heavier than the odd-parity multiplet in all approximations.

Abstract

We calculate the energies of three-quark states with definite permutation symmetry (i.e. of SU(6) multiplets) in the N=0,1,2 shells, confined by the Y-string three-quark potential. The exact Y-string potential consists of one, so-called three-string term, and three angle-dependent two-string terms. Due to this technical complication we treat the problem at three increasingly accurate levels of approximation: 1) the (approximate) three-string potential expanded to first order in trigonometric functions of hyper-spherical angles; 2) the (approximate) three-string potential to all orders in the power expansion in hyper-spherical harmonics, but without taking into account the transition(s) to two-string potentials; 3) the exact minimal-length string potential to all orders in power expansion in hyper-spherical harmonics, and taking into account the transition(s) to two-string potentials. We show the general trend of improvement %convergence of these approximations: The exact non-perturbative corrections to the total energy are of the order of one per cent, as compared with approximation 2), yet the exact energy differences between the $[20,1^{+}], [70,2^{+}], [56,2^{+}], [70,0^{+}]$-plets are shifted to 2:2:0.9, from the Bowler and Tynemouth separation rule 2:2:1, which is obeyed by approximation 2) at the one per cent level. The precise value of the energy separation of the first radial excitation ("Roper") $[56^{\prime},0^{+}]$-plet from the $[70,1^{-}]$-plet depends on the approximation, but does not become negative, i.e. the "Roper" remains heavier than the odd-parity $[70,1^{-}]$-plet in all of our approximations.