Precision thrust cumulant moments at N[superscript 3]LL
Name
Abbate-2012-Precision thrust cumulant moments at N3LL.pdf
Size
2.58 MB
Format
Adobe PDF
Checksum (MD5)
75f8ace544fd9438a5bd52ffbc07f96a
Author(s) • • • •
Abbate, Riccardo
Barreda, Vicent Mateu
Stewart, Iain W.
Fickinger, Michael
Hoang, Andre H.
Date Issued
November 2012
Journal
Physical Review D
Publisher
American Physical Society
Citation
Abbate, Riccardo et al. “Precision thrust cumulant moments at N[superscript 3]LL.” Physical Review D 86.9 (2012). © 2012 American Physical Society
Version
Final published version
Abstract
We consider cumulant moments (cumulants) of the thrust distribution using predictions of the full spectrum for thrust including O(α[subscript s][superscript 3]) fixed order results, resummation of singular N[superscript 3]LL logarithmic contributions, and a class of leading power corrections in a renormalon-free scheme. From a global fit to the first thrust moment we extract the strong coupling and the leading power correction matrix element Ω[subscript 1]. We obtain α[subscript s](m[subscript Z])=0.1140±(0.0004)[subscript exp]±(0.0013)[subscript hadr]±(0.0007)[subscript pert], where the 1-σ uncertainties are experimental, from hadronization (related to Ω[subscript 1]) and perturbative, respectively, and Ω[subscript 1]=0.377±(0.044)exp±(0.039)pert GeV. The nth thrust cumulants for n≥2 are completely insensitive to Ω[subscript 1], and therefore a good instrument for extracting information on higher order power corrections, Ω[subscript [′ over n]/Q[superscript n], from moment data. We find ([bar over Ω]˜[subscript [′ over 2]])[superscript 1/2]=0.74±(0.11)[subscript exp]±(0.09)[subscript pert] GeV.
MIT Department
Massachusetts Institute of Technology. Center for Theoretical Physics
Massachusetts Institute of Technology. Department of Physics
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
DOI of Published Version
https://doi.org/10.1103/PhysRevD.86.094002