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NNLO QCD corrections in full colour for jet production observables at the LHC

Chen, X.; Gehrmann, T.; Glover, E.W.N.; Huss, A.; Mo, J.

NNLO QCD corrections in full colour for jet production observables at the LHC Thumbnail


Authors

X. Chen

T. Gehrmann

A. Huss

J. Mo



Abstract

Calculations for processes involving a high multiplicity of coloured particles often employ a leading colour approximation, where only the leading terms in the expansion of the number of colours Nc and the number of flavours nf are retained. This approximation of the full colour result is motivated by the 1/N2 c suppression of the first subleading terms and by the increasing complexity of including subleading colour contributions to the calculation. In this work, we present the calculations using the antenna subtraction method in the NNLOjet framework for the NNLO QCD corrections at full colour for several jet observables at the LHC. The single jet inclusive cross section is calculated doubly differential in transverse momentum and absolute rapidity and compared with the CMS measurement at 13 TeV. A calculation for dijet production doubly differential in dijet mass and rapidity difference is also performed and compared with the ATLAS 7 TeV data. Lastly, a triply differential dijet cross section in average transverse momentum, rapidity separation and dijet system boost is calculated and compared with the CMS 8 TeV data. The impact of the subleading colour contributions to the leading colour approximation is assessed in detail for all three types of observables and as a function of the jet cone size. The subleading colour contributions play a potentially sizable role in the description of the triply differential distributions, which probe kinematical configurations that are not easily accessed by any of the other observables.

Citation

Chen, X., Gehrmann, T., Glover, E., Huss, A., & Mo, J. (2022). NNLO QCD corrections in full colour for jet production observables at the LHC. Journal of High Energy Physics, 2022(9), Article 25. https://doi.org/10.1007/jhep09%282022%29025

Journal Article Type Article
Acceptance Date Aug 6, 2022
Online Publication Date Sep 5, 2022
Publication Date 2022-09
Deposit Date Sep 6, 2022
Publicly Available Date Sep 6, 2022
Journal Journal of High Energy Physics
Print ISSN 1126-6708
Publisher Scuola Internazionale Superiore di Studi Avanzati (SISSA)
Peer Reviewed Peer Reviewed
Volume 2022
Issue 9
Article Number 25
DOI https://doi.org/10.1007/jhep09%282022%29025

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.





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