Please use this identifier to cite or link to this item: https://hdl.handle.net/20.500.11851/12684
Title: Energy Scale and Resolution for Anti-kt Jets with Radius Parameters R=0.2 and 0.6 Measured in proton-proton Collisions at S=13 TeV with the ATLAS Detector
Authors: Zwalinski, Lukasz
Zou, W.
Zormpa, Olga
Zorbas, T. G.
Zoch, Knut
Zoccoli, Antonio
Zimine, N. I.
Keywords: Astrophysics
Bosons
Colliding Beam Accelerators
Fighter Aircraft
Germanium Compounds
Hadrons
Microstrip Devices
Platinum
Quantum Theory
Tellurium Compounds
Angular Scale
ATLAS Detectors
Energy Resolutions
Energy Scale
Hadronic Decays
Jet Energy
Measurements of
Monte Carlo's Simulation
Proton Proton Collisions
Quantum Chromodynamics
Intelligent Systems
Monte Carlo Methods
Publisher: Springer Nature
Abstract: Jets with different radius parameters R are an important tool for probing quantum chromodynamics processes at different angular scales. Jets with small R=0.2 are instrumental in measurements of the substructure of large-R jets resulting from collimated hadronic decays of energetic W, Z, and Higgs bosons, top quarks, and of potential new resonances. This paper presents measurements of the energy scale, resolution, and associated uncertainties of jets with radius parameters R=0.2 and 0.6, obtained using the ATLAS detector. The results are based on 37fb-1 of proton–proton collision data from the Large Hadron Collider at a centre-of-mass energy of s=13 TeV. A new in situ method for measuring jet energy scale differences between data and Monte Carlo simulations is presented. The systematic uncertainties in the jet energy scale for central jets (|η|<1.2) typically vary from 1% to about 5% as a function of |η| at very low transverse momentum, pT, of around 20 GeV for both R=0.2 and 0.6 jets. The relative energy resolution ranges from (35±6)% at pT=20 GeV to (6±0.5)% at pT=300 GeV for central R=0.2 jets, and is found to be slightly worse for R=0.6 jets. Finally, the effect of close-by hadronic activity on the jet energy scale is investigated and is found to be well modelled by the ATLAS Monte Carlo simulations. © 2025 Elsevier B.V., All rights reserved.
URI: https://doi.org/10.1140/epjc/s10052-025-14226-6
https://hdl.handle.net/20.500.11851/12684
ISSN: 1434-6044
1434-6052
Appears in Collections:Scopus İndeksli Yayınlar Koleksiyonu / Scopus Indexed Publications Collection

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