English

Renormalon-based resummation for spacelike and timelike QCD quantities whose perturbation expansion has general form

High Energy Physics - Phenomenology 2026-02-25 v2 High Energy Physics - Theory

Abstract

We present a generalisation of our previous approach of a renormalon-motivated resummation of the QCD observables. Previously it was applied to the spacelike observables whose perturbation expansion was D(Q2)=a(Q2)+O(a2)D(Q^2) = a(Q^2) + O(a^2), where a(Q2)αs(Q2)/πa(Q^2) \equiv \alpha_s(Q^2)/\pi is the running QCD coupling. Now we generalise the resummation to spacelike quantities D(Q2)=a(Q2)ν0+O(aν0+1)D(Q^2) = a(Q^2)^{\nu_0} + O(a^{\nu_0+1}) and timelike quantities F(σ)=a(σ)ν0+O(aν0+1)F(\sigma) = a(\sigma)^{\nu_0} + O(a^{\nu_0+1}), where ν0\nu_0 is in general a noninteger number (0<ν010<\nu_0 \leq 1). We evaluate with this approach a timelike quantity, namely the scheme-invariant factor of the Wilson coefficient of the chromomagnetic operator in the heavy-quark effective Lagrangian, and related quantities.

Keywords

Cite

@article{arxiv.2509.09042,
  title  = {Renormalon-based resummation for spacelike and timelike QCD quantities whose perturbation expansion has general form},
  author = {Cesar Ayala and Gorazd Cvetič and Reinhart Kögerler},
  journal= {arXiv preprint arXiv:2509.09042},
  year   = {2026}
}

Comments

v2: 39 pp, 7 figures; final version as published in JPG; added references; improved text; new appendix (D) added

R2 v1 2026-07-01T05:31:08.546Z