English

Monte Carlo Top Quark Mass Calibration

High Energy Physics - Phenomenology 2018-03-07 v1

Abstract

The most precise top quark mass measurements use kinematic reconstruction methods, determining the top mass parameter of a Monte Carlo event generator, mtMCm_t^{\rm MC}. Due to the complicated interplay of hadronization and parton shower dynamics in Monte Carlo event generators relevant for kinematic reconstruction, relating mtMCm_t^{\rm MC} to field theory masses is a non-trivial task. In this talk we report on a calibration procedure to determine this relation using hadron level QCD predictions for 2-Jettiness in e+ee^+e^- annihilation, an observable which has kinematic top mass sensitivity and a close relation to the invariant mass of the particles coming from the top decay. The theoretical ingredients of the QCD prediction are reviewed. Fitting e+ee^+e^- 2-Jettiness calculations at NLL/NNLL order to PYTHIA 8.205, we find that mtMCm_t^{\rm MC} agrees with the MSR mass mt,1GeVMSRm_{t,1\,{\rm GeV}}^{\rm MSR} within uncertainties. At NNLL we find mtMC=mt,1GeVMSR+(0.18±0.22)GeVm_t^{\rm MC} = m_{t,1\,{\rm GeV}}^{\rm MSR} + (0.18 \pm 0.22)\,{\rm GeV}. mtMCm_t^{\rm MC} can differ from the pole mass mtpolem_t^{\rm pole} by up to 600MeV600\,{\rm MeV}, and using the pole mass generally leads to larger uncertainties. At NNLL we find mtMC=mtpole+(0.57±0.28)GeVm_t^{\rm MC} = m_t^{\rm pole} + (0.57 \pm 0.28)\,{\rm GeV} as the fit result. In contrast, converting mt,1GeVMSRm_{t,1\,{\rm GeV}}^{\rm MSR} obtained at NNLL to the pole mass gives a result for mtpolem_t^{\rm pole} that is substantially larger and incompatible with the fit result. We also explain some theoretical aspects relevant for employing the C-parameter as an alternative calibration observable.

Keywords

Cite

@article{arxiv.1803.02321,
  title  = {Monte Carlo Top Quark Mass Calibration},
  author = {Bahman Dehnadi and André H. Hoang and Vicent Mateu and Moritz Preisser and Iain W. Stewart},
  journal= {arXiv preprint arXiv:1803.02321},
  year   = {2018}
}

Comments

Talk presented at the 13th International Symposium on Radiative Corrections (RADCOR 2017), St. Gilgen, Austria, 24-29 September 2017. 7 pages, 1 figure