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XXX-th International Workshop on High Energy Physics “Particle and Astroparticle Physics, Gravitation and Cosmology: Predictions, Observations and New Projects”

23–27 Jun 2014
IHEP, Protvino, Theoretical Division
Europe/Moscow timezone

Scientific secretary

Session

Neutrino physics

26 Jun 2014, 15:50
Conference Hall (IHEP, Protvino, Theoretical Division)

Conference Hall

IHEP, Protvino, Theoretical Division

National Research Centre "Kurchatov Institute" Institute for High Energy Physics, Theoretical Division 142281, pl. Nauki, Protvino, Moscow Region, Russian Federation

Description

Neutrino mixing, experiments, models

Presentation materials

There are no materials yet.

  1. 44. Hyper-Kamiokande project
    Dr Akira Konaka Konaka (TRIUMF)
    26/06/2014, 15:50
  2. 45. Detection of supernova neutrinos in Super-Kamiokande
    Motoyasu Ikeda (Kyoto University)
    26/06/2014, 16:15
  3. 46. Recent results from OPERA: search for $\nu_{\mu} \to \nu_{\tau}$ oscillations
    Takuya Omura (Nagoya University)
    26/06/2014, 16:35
    Presentation
    The OPERA experiment aims at providing a direct proof of the $\nu_{\mu} \to \nu_{\tau}$ oscillations by observing $\nu_{\tau}$ CC interactions in an almost pure $\nu_{\mu}$ accelerator beam, the CNGS (CERN Neutrinos to Gran Sasso). The beam exposure started in 2008 and ended in 2012. Events recorded in the Emulsion Cloud Chamber detectors, made of lead plates and nuclear emulsions, are...
  4. 86. Search for nu_mu -> nu_e oscillations with the OPERA experiment
    Svetlana Zemskova (JINR)
    26/06/2014, 16:55
    Presentation
    The main goal of the OPERA experiment is the direct observation of $\nu_{\mu} \to \nu_{\tau}$ oscillations in the appearance mode in the quasi pure $\nu_{\mu}$ CNGS beam. Profiting of the tracking capabilities of the OPERA active target it is possible to detect and reconstruct $\nu_e$ interactions and, therefore, study the subdominant $\nu_{\mu} \to \nu_e$ oscillation channel. Current...
  5. 47. Search for heavy neutrino in the K+ -> mu+ nu_H decay
    Artur Shaikhiev (Russian Academy of Sciences (RU))
    26/06/2014, 17:15
  6. 48. NOvA neutrino experiment
    Filip Jediny (CTU, Praha)
    26/06/2014, 17:55
    Presentation
    The NOvA experiment is a long base-line accelerator based neutrino oscillation experiment. It uses the upgraded NuMI beam from Fermilab and measures electron neutrino appearance and muon neutrino disappearance at its far detector in Ash River, Minnesota. Goals of the experiment include measurements of theta13, mass hierarchy and the CP violating phase. NOvA has begun to take neutrino data and...
  7. 49. ANTARES results
    Evgeny Shirokov (MSU, Moscow)
    26/06/2014, 18:15
  8. 75. KM3NeT project
    Oleg Kalekin (University of Erlangen)
    26/06/2014, 18:35
    Presentation
    The KM3NeT collaboration aims at the construction of a multi-cubic-kilometre scale neutrino telescope in the Mediterranean Sea. The main goal of KM3NeT is to observe high-energy cosmic neutrinos. The first phase of the telescope construction has started at two sites in the Mediterranean: KM3NeT-Fr and KM3NeT-It. The KM3NeT-Fr site is close to that of Antares, about 45 km off-shore Toulon,...
  9. 50. On the flavor composition of the high energy neutrino events in IceCube
    Sergio Palomares-Ruiz (Unknown)
    26/06/2014, 18:55
  10. 85. The recent results of the Daya Bay Experiment
    Mr Bedrich Roskovec (IPNP, Charles University, Prague)
    26/06/2014, 19:15
    Presentation
    The Daya Bay Experiment measured reactor anti-neutrino disappearance on short baseline with unprecedented precision. In a three-neutrino framework our best fit for oscillation parameters is $\sin^22\theta_{13}=0.084\pm0.005$ and $|\Delta m_{ee}^2|=2.44^{+0.10}_{-0.11}\times 10^{-3}\:\text{eV}^2$. We also preformed largely independent measurement of $\theta_{13}$ using neutron capture on...
  11. 51. Panel discussion on Neutrino physics
    26/06/2014, 19:35
    Moderator: Vladimir Obraztsov Panelists: Akira Konaka, Motoyasu Ikeda, Filip Jediny, Evgeny Shirokov, Oleg Kalekin, Sergio Palomares-Ruiz Questions: 1. Can sidereal time analysis of the long time neutrino observations give information about the galaxy distribution in the Local Universe? 2. How well do we need to know the PMNS matrix elements ? 3. Is the existence of MSW effect...
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