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Optimisation of large-radius jet reconstruction for the ATLAS detector in 13 TeV proton-proton collisions
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).ORCID iD: 0000-0002-9766-2670
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).ORCID iD: 0000-0002-3380-8167
Stockholm University, Faculty of Science, Department of Physics.
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Number of Authors: 29262021 (English)In: European Physical Journal C, ISSN 1434-6044, E-ISSN 1434-6052, Vol. 81, no 4, article id 334Article in journal (Refereed) Published
Abstract [en]

Jet substructure has provided new opportunities for searches and measurements at the LHC, and has seen continuous development since the optimization of the large-radius jet definition used by ATLAS was performed during Run 1. A range of new inputs to jet reconstruction, pile-up mitigation techniques and jet grooming algorithms motivate an optimisation of large-radius jet reconstruction for ATLAS. In this paper, this optimisation procedure is presented, and the performance of a wide range of large-radius jet definitions is compared. The relative performance of these jet definitions is assessed using metrics such as their pileup stability, ability to identify hadronically decaying W bosons and top quarks with large transverse momenta. A new type of jet input object, called a 'unified flow object' is introduced which combines calorimeter- and inner-detector-based signals in order to achieve optimal performance across a wide kinematic range. Large-radius jet definitions are identified which significantly improve on the current ATLAS baseline definition, and their modelling is studied using pp collisions recorded by the ATLAS detector at TeV during 2017.

Place, publisher, year, edition, pages
2021. Vol. 81, no 4, article id 334
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Physical Sciences
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URN: urn:nbn:se:su:diva-194345DOI: 10.1140/epjc/s10052-021-09054-3ISI: 000641660400005OAI: oai:DiVA.org:su-194345DiVA, id: diva2:1571705
Available from: 2021-06-23 Created: 2021-06-23 Last updated: 2022-02-25Bibliographically approved

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Andrean, Stefio Y.Backman, FilipBarranco Navarro, LauraBohm, ChristianClement, ChristopheHellman, StenKastanas, AlexandrosLou, XuanhongMilstead, David A.Moa, TorbjörnNelson, Michael E.Pasuwan, PatrawanPereira Sanchez, LauraShaikh, Nabila W.Silverstein, Samuel B.Sjölin, JörgenStrandberg, SaraStrübig, AntoniaValdés Santurio, EduardoWallängen, Veronica

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Andrean, Stefio Y.Backman, FilipBarranco Navarro, LauraBohm, ChristianClement, ChristopheHellman, StenKastanas, AlexandrosLou, XuanhongMilstead, David A.Moa, TorbjörnNelson, Michael E.Pasuwan, PatrawanPereira Sanchez, LauraShaikh, Nabila W.Silverstein, Samuel B.Sjölin, JörgenStrandberg, SaraStrübig, AntoniaValdés Santurio, EduardoWallängen, Veronica
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Department of PhysicsThe Oskar Klein Centre for Cosmo Particle Physics (OKC)
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