Abstract

The measurement of the arrival time of a particle, such as a lepton, a photon, or a pion, reaching the detector provides valuable information. A similar measurement for a hadronic final state, however, is much more challenging as one has to extract the relevant information from a collection of particles. In this paper, we explore various possibilities in defining the time of a jet through the measurable arrival times of the jet constituents. We find that a definition of jet time based on a transverse momentum weighted sum of the times of the constituents has the best performance. For prompt jets, the performance depends on the jet trajectory. For delayed jets, the performance depends on the trajectory of the jet, the trajectory of the mother particle, and the location of the displaced vertex. Compared to the next-best-performing jet time definition, the transverse momentum weighted sum has roughly a factor of ten times better jet time resolution. We give a detailed discussion of the relevant effects and characterize the full geometrical dependence of the performance. These results highlight the critical importance of using a proper definition of jet time with its corresponding detector-dependent calibration and the exciting possibility of deepening our understanding of jets in the time domain.

Details

Title
Jet timing
Author
Chiu Wen Han 1   VIAFID ORCID Logo  ; Liu, Zhen 2   VIAFID ORCID Logo  ; Low, Matthew 3 ; Lian-Tao, Wang 4 

 University of Chicago, Department of Physics, Chicago, USA (GRID:grid.170205.1) (ISNI:0000 0004 1936 7822) 
 University of Minnesota, School of Physics and Astronomy, Minneapolis, USA (GRID:grid.17635.36) (ISNI:0000000419368657) 
 Theoretical Physics Department, Fermilab, Batavia, USA (GRID:grid.417851.e) (ISNI:0000 0001 0675 0679) 
 University of Chicago, Department of Physics, Chicago, USA (GRID:grid.170205.1) (ISNI:0000 0004 1936 7822); University of Chicago, Enrico Fermi Institute, Chicago, USA (GRID:grid.170205.1) (ISNI:0000 0004 1936 7822); University of Chicago, Kavli Institute for Cosmological Physics, Chicago, USA (GRID:grid.170205.1) (ISNI:0000 0004 1936 7822) 
Publication year
2022
Publication date
Jan 2022
Publisher
Springer Nature B.V.
e-ISSN
10298479
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2617112243
Copyright
© The Author(s) 2022. This work is published under CC-BY 4.0 (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.