IR-improved DGLAP parton shower effects for associated production of a W boson and jets in pp collisions at s = 8 and 13 TeV

Author:

Shakerin B.1,Ward B. F. L.1

Affiliation:

1. Physics Department, Baylor University, Waco, TX 76798-7316, USA

Abstract

In a previous paper, hereafter referred to as I, we have analyzed the 7 TeV LHC data on [Formula: see text] events from the standpoint of IR-improved DGLAP parton shower effects, using the IR-improved Herwiri1.031 parton shower MC in comparison with the Herwig6.5 parton shower MC in the context of the exact [Formula: see text] matrix element matched parton shower framework provided by MG5_aMC@NLO. In this paper, we extend this analysis to the LHC 8 and 13 TeV data to investigate the energy dependence of the results obtained in I. Specifically, [Formula: see text] events are generated in the MADGRAPH5_aMC@NLO framework and showered by HERWIG6.521 and HERWIRI1.031 with [Formula: see text] and 0 GeV, respectively. The differential cross sections are reported as functions of jet multiplicity, transverse linear momenta [Formula: see text], the jet pseudorapidity [Formula: see text] and the scalar sum of jet transverse momenta [Formula: see text] for different jet multiplicities 1–3. The dijet cross sections as functions of transverse linear momenta, invariant mass of the dijet and the jet separation are shown as well. Distributions of angular correlations between the jets and the muon are examined as well and the corresponding cross sections are presented. The respective measured cross sections are compared with the exact next-to-leading-order (NLO) matrix element matched parton shower theoretical predictions provided by MADGRAPH5_aMC@NLO/HERWIRI1.031 [Formula: see text] and MADGRAPH5_aMC@NLO/HERWIG6.521 [Formula: see text] and the phenomenological consequences are discussed with an eye toward their energy dependence.

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

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