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TMEX 2018 WCP: European Workshop on Water Cherenkov Precision Detectors for Neutrino and Nucleon Decay Physics

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Centre for Innovation and Technology Transfer Management (Warsaw University of Technology)

Centre for Innovation and Technology Transfer Management

Warsaw University of Technology

Rektorska street 4, 00-614 Warsaw.
Participants
  • Adam Para
  • Anna Dąbrowska
  • Annarita Margiotta
  • Arkadiusz Bubak
  • Beata Kowal
  • Benjamin Richards
  • Carlos Peña Garay
  • Cezary Juszczak
  • Cristovao Vilela
  • David Bravo Berguño
  • David Wark
  • Evangelia Drakopoulou
  • Ewa Rondio
  • Federico Sanchez
  • Gianfranca De Rosa
  • Hide-Kazu TANAKA
  • Jan Kisiel
  • Jan Sobczyk
  • Javier Perez Perez
  • Joanna Zalipska
  • Juan-Pablo Yanez
  • Justyna Lagoda
  • Kamil Porwit
  • Kamil Skwarczyński
  • Karolina Rozwadowska
  • Katarzyna Frankiewicz
  • Katarzyna Kowalik
  • Kenny Chun Yu Ng
  • Luis Labarga
  • Magdalena Posiadala-Zezula
  • Makoto Miura
  • Marcela Batkiewicz
  • Marcin Ziembicki
  • Marek Walczak
  • MEGHNA KUNHIKANNAN KANNICHANKANDY
  • Mirco Hünnefeld
  • Nuno Barros
  • Piotr Kalaczyński
  • Piotr Mijakowski
  • Spencer Axani
  • Sunny Seo
  • TAKASHI KOBAYASHI
  • Thomas Kintscher
  • Tomasz Wachala
  • Tsuyoshi NAKAYA
  • Vittorio Paolone
  • Wojciech Żurek
  • Yasuhiro NISHIMURA
  • Yasuo Takeuchi
  • Yousuke Kataoka
  • Yuuki Nakano
  • Zepeng Li
  • Wednesday, 19 September
    • 09:00 → 10:00
      Introductory talks
    • 10:00 → 10:25
      Coffee break 25m
    • 10:25 → 12:20
      Current WC running experiments
    • 12:20 → 13:40
      Lunch 1h 20m
    • 13:40 → 14:15
      Current WC running experiments Centre for Innovation and Technology Transfer Management

      Centre for Innovation and Technology Transfer Management

      Warsaw University of Technology

      Rektorska street 4, 00-614 Warsaw.
      • 13:40
        Status and prospects of the Antares and KM3NeT experiments 35m

        The ANTARES detector is the first undersea neutrino telescope. It has been taking data continuously since 2007, with the main goal of searching for astrophysical neutrinos in the TeV-PeV range.

        The optical properties of the sea water, in particular the long scattering length, allow for a very good resolution in the reconstruction of the interaction vertex for neutrinos of all flavours and in the identification of neutrino direction. Its location in the Northern hemisphere guarantees an excellent point of view for the identification of neutrino sources located in the Southern Sky, with a special attention to the Galactic Plane and Centre.

        The observations performed with ANTARES have allowed to put constraints on the origin of the cosmic neutrino flux discovered by the IceCube detector. Moreover, the ANTARES Collaboration is actively involved into a manifold multi-messenger program. In this contribution, the latest experimental results on the searches for neutrinos correlated with the recently discovered gravitational wave signals and FRB events will be discussed. Also the results on indirect searches for dark matter from massive objects like the Sun and the Galactic Center will be presented.

        The high quality of the data collected with the ANTARES telescope and the competitiveness of the results have proven the tremendous potential of the sea water Cherenkov technique, paving the way to the new, larger telescope, KM3NeT.
        KM3NeT is a research infrastructure hosting neutrino telescopes in the Mediterranean Sea. Two detectors using the same detection technology but different granularity are foreseen: ARCA, with an instrumented volume of a km3, at a depth of 3500 m offshore Capo Passero, Italy, designed to discover and observe high-energy neutrinos (TeV ÷ PeV) of cosmic origin, increasing the potential of the ANTARES telescope in the identification of neutrino sources; and ORCA, with an instrumented volume of a few Mton, at a depth of 2500 m offshore Toulon, France, optimized to measure atmospheric neutrinos with energies at the GeV scale, with the goal to study of the neutrinos mass hierarchy.

        The KM3NeT Collaboration has started the construction of both detectors. The first detection units were deployed and analyses are ongoing to validate the detector performances. The status of the ARCA and ORCA detectors and the future prospects of the project will be presented.

        Speaker: Annarita Margiotta
        TMEX_warsaw_margiotta.pdf
    • 14:15 → 15:15
      Neutrino interactions
      • 14:15
        Theory landscape of neutrino interactions 35m
        Speaker: Federico Sanchez
        CrossSectionsTMEX.pdf
      • 14:50
        Neutrino generators: NuWro, NEUT, GENIE 25m
        Speaker: Cezary Juszczak
        juszczak-2018.pdf
    • 15:15 → 15:40
      Coffee break 25m
    • 15:40 → 17:20
      Detection techniques, particle reconstruction
    • 17:20 → 17:40
      Announcements 20m Centre for Innovation and Technology Transfer Management

      Centre for Innovation and Technology Transfer Management

      Warsaw University of Technology

      Rektorska street 4, 00-614 Warsaw.
      announcements.pdf Hera_Hotel_walk_to_venue.pdf
  • Thursday, 20 September
    • 09:20 → 10:10
      Current WC running experiments
      • 09:20
        Reducing interaction model uncertainties in long baseline oscillation measurements with the J-PARC E61 experiment 25m
        Speaker: Cristovao Vilela
        cvilela_TMEX2018_JPARC_E61.pdf
      • 09:45
        ANNIE Phase II 25m
        Speaker: Evangelia Drakopoulou
        ANNIE_TMEXSep2018.pdf
    • 10:10 → 10:45
      Photosensors and front-end electronics Centre for Innovation and Technology Transfer Management

      Centre for Innovation and Technology Transfer Management

      Warsaw University of Technology

      Rektorska street 4, 00-614 Warsaw.
    • 10:45 → 11:10
      Coffee break 25m
    • 11:10 → 11:45
      Photosensors and front-end electronics
      • 11:10
        Multi-PMT units for the Water Cherenkov detectors, the case of KM3Net and its evolution for E61 and Hyper-Kamiokande 35m
        Speaker: Gianfranca de Rosa
        GDeRosa-TMEX2018 (1).pdf
    • 11:45 → 12:35
      Electronics/DAQ
    • 12:35 → 13:55
      Lunch 1h 20m
    • 13:55 → 14:20
      Electronics/DAQ
    • 14:20 → 15:20
      Civil engineering
    • 15:20 → 15:45
      Coffee break 25m
    • 15:45 → 16:30
      Water or ice
    • 16:30 → 19:30
      Bus tour
    • 19:30 → 22:00
      Dinner: Dinner at Restaurant Wilcza 50
  • Friday, 21 September
    • 09:00 → 09:30
      Physics results with WC experiments: Nucleon decay
    • 09:30 → 10:35
      Physics results with WC experiments: Astrophysics
    • 10:35 → 11:00
      Coffee break 25m
    • 11:00 → 12:00
      Physics results with WC experiments: Astrophysics
    • 12:00 → 12:40
      Physics results with WC experiments: Neutrino oscillation
      • 12:00
        Theory-landscape and the place of WC detectors in neutrino oscillation studies (including global fits) 40m
        Speaker: Carlos Peña-Garay (LSC, IFIC-UV)
        6_nuth_TMEX.pdf
    • 12:40 → 14:05
      Lunch 1h 25m
    • 14:05 → 15:35
      Physics results with WC experiments: Neutrino oscillation
    • 15:35 → 15:55
      Coffee break 20m
    • 15:55 → 16:25
      Physics results with WC experiments: Neutrino oscillation
      • 15:55
        Recent osc. results from T2K and NoVa 30m
        Speaker: Vittorio Paolone (University of Pittsburgh)
        T2K_TMEX2018_.pdf
    • 16:25 → 17:35
      Closing remarks
      • 16:25
        Future Outlook and Summary 40m
        Speaker: Tsuyoshi Nakaya
      • 17:05
        Discussion 30m
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