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Power corrections in the dispersive model for a determination of the strong coupling constant from the thrust distribution

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abstract

In the context of the dispersive model for non-perturbative corrections, we extend the leading renormalon subtraction to NNLO for the thrust distribution in $e^+e^-$ annihilation. Within this framework, using a NNLL+NNLO perturbative description and including bottom quark mass effects to NLO, we analyse data in the centre-of-mass energy range $\sqrt{s}=14-206$ GeV in view of a simultaneous determination of the strong coupling constant and the non-perturbative parameter $\alpha_0$. The fits are performed by matching the resummed and fixed-order predictions both in the R and the log-R matching schemes. The final values in the R scheme are $\alpha_s(M_Z) = 0.1131^{+0.0028}_{-0.0022}$, $\alpha_0(2 {\rm GeV}) = 0.538^{+0.102}_{-0.047}$.

fields

hep-ph 1

years

2026 1

verdicts

UNVERDICTED 1

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Centauric 1-Jettiness in DIS and Universal Power Corrections

hep-ph · 2026-06-18 · unverdicted · novelty 7.0

Introduces Centauric 1-jettiness in DIS, derives N3LL resummation matched to NLO, and establishes universal non-perturbative power corrections scaling as 1/R via reduction to rescaled hemisphere soft function.

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  • Centauric 1-Jettiness in DIS and Universal Power Corrections hep-ph · 2026-06-18 · unverdicted · none · ref 17 · internal anchor

    Introduces Centauric 1-jettiness in DIS, derives N3LL resummation matched to NLO, and establishes universal non-perturbative power corrections scaling as 1/R via reduction to rescaled hemisphere soft function.