Conveners
WG1: Present and near future oscillation experiments
- Takeshi Nakadaira (KEK)
- Alexandre Sousa (University of Cincinnati)
- Enrique Fernandez-Martinez (Universidad Autonoma de Madrid)
WG1: Proposals for next generation oscillation facilities I
- Alexandre Sousa (University of Cincinnati)
- Takeshi Nakadaira (KEK)
- Enrique Fernandez-Martinez (Universidad Autonoma de Madrid)
WG1: Proposals for next generation oscillation facilities II
- Alexandre Sousa (University of Cincinnati)
- Takeshi Nakadaira (KEK)
- Enrique Fernandez-Martinez (Universidad Autonoma de Madrid)
WG1: Mass hierarchy determination I
- Alexandre Sousa (University of Cincinnati)
- Takeshi Nakadaira (KEK)
- Enrique Fernandez-Martinez (Universidad Autonoma de Madrid)
WG1: Mass hierarchy determination II
- Takeshi Nakadaira (KEK)
- Alexandre Sousa (University of Cincinnati)
- Enrique Fernandez-Martinez (Universidad Autonoma de Madrid)
WG1: Neutrinoless double beta decay
- Takeshi Nakadaira (KEK)
- Alexandre Sousa (University of Cincinnati)
- Enrique Fernandez-Martinez (Universidad Autonoma de Madrid)
WG1: Sterile neutrinos and reactor oscillation results
- Takeshi Nakadaira (KEK)
- Enrique Fernandez-Martinez (Universidad Autonoma de Madrid)
- Alexandre Sousa (University of Cincinnati)
WG1: Summary preparation
- Takeshi Nakadaira (KEK)
- Alexandre Sousa (University of Cincinnati)
- Enrique Fernandez-Martinez (Universidad Autonoma de Madrid)
Description
Nu Oscillation Physics
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DrJonathan Paley(Argonne National Laboratory)
20/08/2013, 10:55
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...
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Prof.Sanjib Kumar Agarwalla(Institute of Physics, Bhubaneswar)
20/08/2013, 11:45
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Alain Blondel(DPNC UNiversity og Geneva)
20/08/2013, 16:40
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...
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Pilar Coloma(Center for Neutrino Physics at Virginia Tech)
21/08/2013, 08:50
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DrRyan Bayes(University of Glasgow)
21/08/2013, 09:10
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...
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DrMattias Blennow(KTH Royal Institute of Techology)
21/08/2013, 09:30
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DrWei Wang(William and Mary)
21/08/2013, 13:30
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...
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Prof.Jarah Evslin(Institute of High Energy Physics, Chinese Academy of Sciences)
21/08/2013, 13:55
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...
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DrKenneth Clark(University of Toronto)
21/08/2013, 14:20
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,...
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DrMattias Blennow(KTH Royal Institute of Technology)
21/08/2013, 14:45
Neutrino Oscillation Physics
To be supplied
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DrSovan Chakraborty(Max-Planck Institute for Physics)
21/08/2013, 16:00
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DrThomas Eberl(Erlangen Centre for Astroparticle Physics)
21/08/2013, 16:20
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.
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Prof.Liang Yang(University of Illinois at Urbana-Champaign)
22/08/2013, 08:30
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DrLopez Pavon Jacobo(SISSA)
22/08/2013, 08:50
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DrToshihiko Ota(Saitama University)
22/08/2013, 09:10
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...
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MrXiaochuan Lu(UC Berkeley)
22/08/2013, 09:30
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MsMaria Archidiacono(Aarhus University)
23/08/2013, 11:30
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MsRalitsa Sharankova(Tokyo Institute of Technology)
23/08/2013, 11:50
23/08/2013, 16:00
