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Driving missing data at the LHC: NNLO predictions for the ratio of γ + j and Z + j

Campbell, John M.; Ellis, R. Keith; Williams, Ciaran

Driving missing data at the LHC: NNLO predictions for the ratio of γ + j and Z + j Thumbnail


Authors

John M. Campbell

Ciaran Williams



Abstract

In this paper, we present a calculation of the γ+j process at next-to-next-to-leading order (NNLO) in QCD and compare the resulting predictions to 8 TeV CMS data. We find good agreement with the shape of the photon pT spectrum, particularly after the inclusion of additional electroweak corrections, but there is a tension between the overall normalization of the theoretical prediction and the measurement. We use our results to compute the ratio of Z(→ℓ+ℓ−)+j to γ+j events as a function of the vector boson transverse momentum at NNLO, a quantity that is used to normalize Z(→νν¯)+j backgrounds in searches for dark matter and supersymmetry. Our NNLO calculation significantly reduces the theoretical uncertainty on this ratio, thus boosting its power for future searches of new physics.

Citation

Campbell, J. M., Ellis, R. K., & Williams, C. (2017). Driving missing data at the LHC: NNLO predictions for the ratio of γ + j and Z + j. Physical Review D, 96(1), Article 014037. https://doi.org/10.1103/physrevd.96.014037

Journal Article Type Article
Acceptance Date Apr 20, 2017
Online Publication Date Jul 31, 2017
Publication Date Jul 31, 2017
Deposit Date Aug 23, 2017
Publicly Available Date Aug 23, 2017
Journal Physical Review D
Print ISSN 2470-0010
Electronic ISSN 2470-0029
Publisher American Physical Society
Peer Reviewed Peer Reviewed
Volume 96
Issue 1
Article Number 014037
DOI https://doi.org/10.1103/physrevd.96.014037
Public URL https://durham-repository.worktribe.com/output/1370707

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Copyright Statement
Reprinted with permission from the American Physical Society: Physical Review D 96, 014037 © 2017 by the American Physical Society. Readers may view, browse, and/or download material for temporary copying purposes only, provided these uses are for noncommercial personal purposes. Except as provided by law, this material may not be further reproduced, distributed, transmitted, modified, adapted, performed, displayed, published, or sold in whole or part, without prior written permission from the American Physical Society.






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