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International Workshop on Neutrino Factories, Super Beams and Beta Beams

19-24 August 2013
IHEP
Asia/Shanghai timezone
Home > Timetable > Session details
PDF | iCal

WG1

Place

Location: IHEP
Room: TBA
Date: from 20 Aug 10:30 to 23 Aug 17:30

Description

Nu Oscillation Physics

Conveners

  • 20 Aug 10:30 - 12:30 PM Present and near future oscillation experiments
    • Prof. Sousa, Alexandre (University of Cincinnati)
    • Dr. Fernandez-Martinez, Enrique (Universidad Autonoma de Madrid)
    • Dr. Nakadaira, Takeshi (KEK)
  • 20 Aug 16:00 - 5:30 PM Proposals for next generation oscillation facilities I
    • Prof. Sousa, Alexandre (University of Cincinnati)
    • Dr. Fernandez-Martinez, Enrique (Universidad Autonoma de Madrid)
    • Dr. Nakadaira, Takeshi (KEK)
  • 21 Aug 08:30 - 10:00 AM Proposals for next generation oscillation facilities II
    • Prof. Sousa, Alexandre (University of Cincinnati)
    • Dr. Fernandez-Martinez, Enrique (Universidad Autonoma de Madrid)
    • Dr. Nakadaira, Takeshi (KEK)
  • 21 Aug 13:30 - 3:30 PM Mass hierarchy determination I
    • Prof. Sousa, Alexandre (University of Cincinnati)
    • Dr. Fernandez-Martinez, Enrique (Universidad Autonoma de Madrid)
    • Dr. Nakadaira, Takeshi (KEK)
  • 21 Aug 16:00 - 5:30 PM Mass hierarchy determination II
    • Prof. Sousa, Alexandre (University of Cincinnati)
    • Dr. Fernandez-Martinez, Enrique (Universidad Autonoma de Madrid)
    • Dr. Nakadaira, Takeshi (KEK)
  • 22 Aug 08:30 - 10:00 AM Neutrinoless double beta decay
    • Prof. Sousa, Alexandre (University of Cincinnati)
    • Dr. Fernandez-Martinez, Enrique (Universidad Autonoma de Madrid)
    • Dr. Nakadaira, Takeshi (KEK)
  • 23 Aug 10:30 - 12:30 PM Sterile neutrinos and reactor oscillation results
    • Prof. Sousa, Alexandre (University of Cincinnati)
    • Dr. Fernandez-Martinez, Enrique (Universidad Autonoma de Madrid)
    • Dr. Nakadaira, Takeshi (KEK)
  • 23 Aug 16:00 - 5:30 PM Summary preparation
    • Prof. Sousa, Alexandre (University of Cincinnati)
    • Dr. Fernandez-Martinez, Enrique (Universidad Autonoma de Madrid)
    • Dr. Nakadaira, Takeshi (KEK)

Timetable | Contribution List

Displaying 34 contributions out of 34
Session: WG1
Presented by Mr. Xiaochuan LU on 22/8/2013 at 1:30
Session: WG1
Track: Neutrino Oscillation Physics
The value of the last mixing angle theta13 has been measured the Daya Bay Reactor Neutrino Experiment, followed by consistent results from RENO and Double Chooz. Its large value, compared with most speculated values before its discovery, creates a unique opportunity in resolving neutrino mass hierarchy (MH) using medium-baseline reactor antineutrino experiments employing massive liquid scintillato ... More
Presented by Dr. Wei WANG on 21/8/2013 at 5:30
Session: WG1
Track: Neutrino Oscillation Physics
Analyses of neutrino mass hierarchy determinations at future experiments determine an expected Delta Chi^2. As the hierarchy is a discrete choice, and not a continuous degree of freedom, this Delta Chi^2 does not obey Wilks' theorem. As a consequence it does not follow a chi^2 distribution and its square root is not the number s of sigmas of confidence that can be expected. I will present a sim ... More
Presented by Prof. Jarah EVSLIN on 21/8/2013 at 5:55
Session: WG1
Presented by Ms. Maria ARCHIDIACONO on 23/8/2013 at 3:30
Session: WG1
Presented by Dr. Soeren JETTER on 23/8/2013 at 4:10
Session: WG1
Track: Neutrino Oscillation Physics
To be supplied
Presented by Dr. Mattias BLENNOW on 21/8/2013 at 6:45
Session: WG1
Presented by Yvonne WONG on 21/8/2013 at 9:00
Session: WG1
Presented by Dr. Sovan CHAKRABORTY on 21/8/2013 at 8:00
Session: WG1
Presented by Ms. Ralitsa SHARANKOVA on 23/8/2013 at 3:50
Session: WG1
Presented by Prof. Karol LANG on 20/8/2013 at 8:00
ESS
Session: WG1
Presented by Dr. Marcos DRACOS on 20/8/2013 at 9:00
Session: WG1
Presented by Dr. Mattias BLENNOW on 21/8/2013 at 1:30
Session: WG1
Presented by paola SALA on 23/8/2013 at 3:10
Session: WG1
Presented by Dr. Sandhya CHOUBEY on 21/8/2013 at 8:40
Session: WG1
Presented by James STRAIT on 20/8/2013 at 8:20
Session: WG1
Track: Neutrino Oscillation Physics
A neutrino factory provides a well defined neutrino beam with a wide range of oscillation channels for the direct detection of CP violation in the neutrino sector. To make use of this beam, a detector must have excellent charge discrimination capabilities because the un-oscillated background has the same flavour, but with the opposite charge to the signal. A magnetic field is required to achi ... More
Presented by Dr. Ryan BAYES on 21/8/2013 at 1:10
Session: WG1
Presented by Dr. Joao COELHO on 20/8/2013 at 2:30
Session: WG1
Session: WG1
Presented by Prof. Kirk T MCDONALD on 21/8/2013 at 7:10
Session: WG1
Presented by Pilar COLOMA on 21/8/2013 at 0:50
Q&A
Session: WG1
Presented by Dr. Paul SOLER
Session: WG1
Presented by Prof. Sanjib Kumar AGARWALLA on 20/8/2013 at 3:45
Session: WG1
Presented by Prof. Liang YANG on 22/8/2013 at 0:30
Session: WG1
Track: Neutrino Oscillation Physics
The NuMI Off-Axis $\nu_e$ Appearance (\nova) experiment, currently under construction, is a long-baseline neutrino oscillation experiment optimized for the measurement of $\nu_\mu \rightarrow \nu_e$ appearance. The experiment consists of two nearly identical fully-active liquid-scintillator tracking calorimeter detectors separated by 810 km and exposed to an upgraded 700 kW NuMI beam from Fermi N ... More
Presented by Dr. Jonathan PALEY on 20/8/2013 at 2:55
Session: WG1
Presented by Dr. Megan FRIEND on 20/8/2013 at 3:20
Session: WG1
Presented by Dr. Lopez Pavon JACOBO on 22/8/2013 at 0:50
Session: WG1
Presented by Prof. Takasumi MARUYAMA on 23/8/2013 at 2:50
Session: WG1
Presented by Dr. Pavlovic ZARKO on 23/8/2013 at 2:30
Session: WG1
Track: Neutrino Oscillation Physics
IceCube and its low energy extension DeepCore have been deployed at the South Pole and taking data since early 2011. DeepCore provides a neutrino energy threshold of about 10 GeV, which allows IceCube to access a rich variety of physics including indirectly searching for WIMP dark matter and studying atmospheric neutrinos. Currently under consideration is a new in-fill array named PINGU, which wi ... More
Presented by Dr. Kenneth CLARK on 21/8/2013 at 6:20
Session: WG1
on 23/8/2013 at 8:00
Session: WG1
If the standard model is an effective model of a fundamental theory realized at high energy scales, the full Lagrangian that describes physics at the electroweak scale should contain the series of higher-dimensional operators whose mass dimensions are higher than four. Such effective interactions suppressed by the inverse power of new physics scale $\Lambda_{NP}$ are typical low-energy remnant of ... More
Presented by Dr. Toshihiko OTA on 22/8/2013 at 1:10
Session: WG1
Presented by Dr. Taku ISHIDA on 21/8/2013 at 0:30
Session: WG1
Track: Neutrino Oscillation Physics
The LAGUNA-LBNO European design study aims at defining a deep underground neutrino observatory for the study of neutrino oscillations at long baselines, the investigation of the Grand Unification of elementary forces and for the detection of known and unknown astrophysical sources of neutrinos. For the neutrino oscillation studies, the project is specifically considering long baseline neutrino bea ... More
Presented by Alain BLONDEL on 20/8/2013 at 16:40
Session: WG1
Track: Neutrino Oscillation Physics
The talk will present the current status of a dedicated feasibility study “Oscillation Research with Cosmics in the Abyss” (ORCA) to evaluate the potential of a neutrino mass hierarchy measurement with “phase 1” of KM3NeT, the future multi-km3 water Cherenkov neutrino telescope in the Mediterranean.
Presented by Dr. Thomas EBERL on 21/8/2013 at 16:20
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