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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