Journal article
NLO QCD predictions for tt¯bb¯¯ production in association with a light jet at the LHC
- Abstract:
- Theoretical predictions for tt¯bb¯¯ production are of crucial importance for tt¯ H measurements in the H → b b¯¯ channel at the LHC. To address the large uncertainties associated with the modelling of extra QCD radiation in tt¯ bb¯¯ events, in this paper we present a calculation of pp → tt¯ bb¯¯ j at NLO QCD. The behaviour of NLO corrections is analysed in a variety of observables, and to assess theoretical uncertainties we use factor- two rescalings as well as different dynamic scales. In this context, we propose a systematic alignment of dynamic scales that makes it possible to disentangle normalisation and shape uncertainties in a transparent way. Scale uncertainties at NLO are typically at the level of 20–30% in integrated cross sections, and below 10% for the shapes of distributions. The kinematics of QCD radiation is investigated in detail, including the effects of its recoil on the objects of the tt¯ bb¯¯ system. In particular, we discuss various azimuthal correlations that allow one to characterise the QCD recoil pattern in a precise and transparent way. In general, the calculation at hand provides a variety of precise benchmarks that can be used to validate the modelling of QCD radiation in tt¯bb¯¯ generators. Moreover, as we will argue, pp → tt¯bb¯¯ j at NLO entails information that can be used to gain insights into the perturbative convergence of the inclusive tt¯bb¯¯ cross section beyond NLO. Based on this idea, we address the issue of the large NLO K-factor observed in σtt¯bb¯, and we provide evidence that supports the reduction of this K-factor through a mild adjustment of the QCD scales that are conventionally used for this process. The presented 2 → 5 NLO calculations have been carried out using OpenLoops 2 in combination with Sherpa and Munich.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 1.6MB, Terms of use)
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- Publisher copy:
- 10.1007/jhep12(2019)015
Authors
- Publisher:
- Springer Verlag
- Journal:
- Journal of High Energy Physics More from this journal
- Volume:
- 2019
- Issue:
- 12
- Article number:
- 15
- Publication date:
- 2019-12-03
- Acceptance date:
- 2019-11-12
- DOI:
- EISSN:
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1029-8479
- ISSN:
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1126-6708
- Language:
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English
- Pubs id:
-
pubs:1077187
- UUID:
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uuid:a2515f32-f5ae-469c-b61b-2d6ba34b2b7b
- Local pid:
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pubs:1077187
- Source identifiers:
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1077187
- Deposit date:
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2019-12-10
- ARK identifier:
Terms of use
- Copyright holder:
- Buccioni et al
- Copyright date:
- 2019
- Notes:
- © The Author(s) 2019. This article is published under an open access license. Please check the 'Copyright Information' section for details of this license and what re-use is permitted. If your intended use exceeds what is permitted by the license or if you are unable to locate the licence and re-use information, please contact the Rights and Permissions team.
- Licence:
- CC Attribution (CC BY)
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