Table of Contents
Fetching ...

Third-order Coulomb corrections to the S-wave Green function, energy levels and wave functions at the origin

M. Beneke, Y. Kiyo, K. Schuller

TL;DR

The paper addresses large higher-order corrections in heavy-quarkonium and top-quark threshold physics by computing third-order (NNNLO) Coulomb corrections to S-wave energy levels, wave functions at the origin, and the Green function within a nonrelativistic QCD framework. It provides analytic expressions for the Coulomb contributions e_i^C and f_i^C (and non-Coulomb pieces e_i^{nC}, f_i^{nC}) for arbitrary n, including new terms such as c_E,3 and c_ψ,3, with Bethe logarithms L_E(n) entering the energy corrections. The results enable a complete S-wave spectrum at order α_s^5, improve the perturbative treatment of bottomonium masses through the PS-mass scheme (e.g., m_b,PS(2 GeV) = 4.57 GeV), and offer controlled predictions for top-quark pair production near threshold with residual Coulomb uncertainties around a few percent. This work lays the groundwork for precise quarkonium spectroscopy and top-threshold phenomenology by clarifying the convergence and scale- dependence of perturbative Coulomb corrections.

Abstract

We obtain analytic expressions for the third-order corrections due to the strong interaction Coulomb potential to the S-wave Green function, energy levels and wave functions at the origin for arbitrary principal quantum number n. Together with the known non-Coulomb correction this results in the complete spectrum of S-states up to order alpha_s^5. The numerical impact of these corrections on the Upsilon spectrum and the top quark pair production cross section near threshold is estimated.

Third-order Coulomb corrections to the S-wave Green function, energy levels and wave functions at the origin

TL;DR

The paper addresses large higher-order corrections in heavy-quarkonium and top-quark threshold physics by computing third-order (NNNLO) Coulomb corrections to S-wave energy levels, wave functions at the origin, and the Green function within a nonrelativistic QCD framework. It provides analytic expressions for the Coulomb contributions e_i^C and f_i^C (and non-Coulomb pieces e_i^{nC}, f_i^{nC}) for arbitrary n, including new terms such as c_E,3 and c_ψ,3, with Bethe logarithms L_E(n) entering the energy corrections. The results enable a complete S-wave spectrum at order α_s^5, improve the perturbative treatment of bottomonium masses through the PS-mass scheme (e.g., m_b,PS(2 GeV) = 4.57 GeV), and offer controlled predictions for top-quark pair production near threshold with residual Coulomb uncertainties around a few percent. This work lays the groundwork for precise quarkonium spectroscopy and top-threshold phenomenology by clarifying the convergence and scale- dependence of perturbative Coulomb corrections.

Abstract

We obtain analytic expressions for the third-order corrections due to the strong interaction Coulomb potential to the S-wave Green function, energy levels and wave functions at the origin for arbitrary principal quantum number n. Together with the known non-Coulomb correction this results in the complete spectrum of S-states up to order alpha_s^5. The numerical impact of these corrections on the Upsilon spectrum and the top quark pair production cross section near threshold is estimated.

Paper Structure

This paper contains 12 sections, 49 equations, 4 figures.

Figures (4)

  • Figure 1: The bottom PS mass, $m_{b,\rm PS}(2\,\hbox{GeV})$, extracted from the experimental value $M_{\Upsilon(1S)}=9.460\,$GeV as a function of renormalization scale $\mu$ at LO (long dashes, black), NLO (long-short dashes, red), NNLO (short dashes, green) and NNNLO (solid, blue).
  • Figure 2: Predicted masses of the $\Upsilon(\rm{2S})$ and $\Upsilon(\rm{3S})$ as a function of the renormalization scale $\mu$. The lines refer to LO (long dashes, black), NLO (long-short dashes, red), NNLO (short dashes, green) and NNNLO (solid, blue). The widths of the bands for the experimental mass values are exaggerated.
  • Figure 3: The Coulomb wave function at the origin squared for the ground state ($n=1$) normalized by $|\Psi_1^{(0)}(0)|^2$ at $\mu_B=32.6\,$GeV is shown as a function of the renormalization scale $\mu$. The input parameters are $m_{t,\rm PS}(20\,\hbox{GeV})=175\,$GeV, $\nu=m_{t,\rm PS} C_F \alpha_s(\mu)$. The lines refer to LO (long dashes, black), NLO (long-short dashes, red), NNLO (short dashes, green) and NNNLO (solid, blue).
  • Figure 4: Top quark pair production cross section (Coulomb corrections only) for $m_{t,\rm PS}=175\,$GeV, $\Gamma_t=1.5\,$GeV. Upper panel: successive approximations up to the third order for $\mu=30\,$GeV. Lower panel: Scale dependence of the third-order approximation. See text for further explanation.