Go to the Indico Home Page Oldest event Older event Up to category Newer event Newest event Printable version
  • Compact style
  • Indico style
  • Indico style - inline minutes
  • Indico style - numbered
  • Indico style - numbered + minutes
  • Indico Weeks View
    • Switch to the management area of this event
    Login

    Work meeting of LHC Darkshowers taskforce

    → Europe/Zurich
    Cesare Cazzaniga, Christiane Scherb, Felix Karl David Kahlhoefer (Karlsruhe Institute of Technology), Jackson Carl Burzynski (University of Oklahoma (US)), Kevin Pedro (Fermi National Accelerator Lab. (US)), Sukanya Sinha (The University of Manchester (GB))
    Description

    If you are interested in contributing to the taskforce, join this mailing list to get meeting updates

    GMT20260615-135957_Recording_1920x1200.mp4
    Contact
    Work meeting of LHC Darkshowers taskforce
    Zoom Meeting ID
    62555445412
    Host
    Sukanya Sinha
    Alternative hosts
    Jackson Carl Burzynski, Cesare Cazzaniga, Annapaola De Cosa, Kevin Pedro
    Useful links
    Join via phone
    Zoom URL
      • 16:00 → 16:10
        Introduction and general news 10m
        Speakers: Cesare Cazzaniga (Deutsches Elektronen-Synchrotron (DE)), Sukanya Sinha (The University of Manchester (GB))

        LHC BSM WG Darkshowers plenary: tomorrow (16th June): https://indico.cern.ch/event/1687390/ [3-5pm CET]

      • 16:10 → 16:30
        Semi-visible jets model 20m
        Speaker: Emily Ann Smith (Fermi National Accelerator Lab. (US))
        DarkShowers Taskforce.pdf
      • 16:30 → 16:50
        Pythia version comparisons 20m
        Speaker: Mr Miguel Angel Avendano Bernal (University of Southampton)
        Dark_Showers_Taskforce_PYcomp_Miguel_Talk_v1 (1).pdf

        We will review different tools at the jet-substructure level to study Semi-Visible Jets (SVJs), formed by the decay of an intermediate massive Z' boson. While characterising these signals, we need to compare how much changes have been through version to version of PYTHIA8. We will show a review at how the HV parameters will vary from signal to signal in each version. The angularity and the charged hadron mutiplicity will help us to understand how the hadronisation and the dark shower has been changed from earlier versions to the latest version. Finally, we will also mention how global kinematics (MET), were modified from version to version.