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Prof. Mark Hartz (Kavli IPMU (WPI), The University of Tokyo/TRIUMF)19/07/2014, 09:00
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Prof. Francesca Di Lodovico (Queen Mary, University of London)19/07/2014, 09:10
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Matthew Malek19/07/2014, 09:15
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Dr David Hadley (University of Warwick)19/07/2014, 09:30
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Dr Mark Rayner (Université de Genève)19/07/2014, 09:50
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Prof. Francesca Di Lodovico (Queen Mary, University of London)19/07/2014, 10:10
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Dr Michael Wilking (TRIUMF)19/07/2014, 10:30
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Dr Mark Scott (TRIUMF)19/07/2014, 11:05
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Dr Morgan Wascko (Imperial College London)19/07/2014, 11:40
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Prof. Masato SHIOZAWA (The University of Tokyo, Institute for Cosmic Ray Research, ICRR)19/07/2014, 13:00
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Dr Takatomi Yano (Kobe Univ.)19/07/2014, 13:20
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Dr Yoshinari Hayato (Kamioka obs., ICRR, Univ. of Tokyo)19/07/2014, 13:40
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19/07/2014, 14:00
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19/07/2014, 14:20
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Dr Akira Konaka (TRIUMF)20/07/2014, 08:30
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Dr Akira Konaka (TRIUMF)20/07/2014, 08:58
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Prof. Jonathan Bagger (TRIUMF)20/07/2014, 09:00
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Prof. Masato SHIOZAWA (The University of Tokyo, Institute for Cosmic Ray Research, ICRR)20/07/2014, 09:10some backgrounds, meeting goals (HK physics, detector design, foreign contributions)Go to contribution page
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Prof. Tsuyoshi NAKAYA (Kyoto)20/07/2014, 09:30
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Tatsuya NAKADA (Ecole Polytechnique Federale de Lausanne (CH))20/07/2014, 09:50
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Prof. Hiroaki AIHARA (University of Tokyo)20/07/2014, 10:10
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Prof. Masashi Yokoyama (University of Tokyo)20/07/2014, 10:50
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Dr Akira Konaka (TRIUMF)20/07/2014, 11:00
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Roger Wendell (ICRR)20/07/2014, 11:15
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Prof. Chris Walter (Duke University), Dr Erin O'Sullivan (Duke University)20/07/2014, 11:25
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Prof. Tsuyoshi NAKAYA (Kyoto)20/07/2014, 11:35
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Prof. Nigel SMITH (SNOLab)20/07/2014, 13:30
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Prof. Dawn Williams (University of Alabama)20/07/2014, 13:50The IceCube Neutrino Observatory, completed in 2010 and located at the geographic South Pole, is the largest neutrino telescope in the world. IceCube includes the more densely instrumented DeepCore subarray, which increases IceCube's sensitivity at neutrino energies down to 10 GeV. DeepCore has recently demonstrated sensitivity to muon neutrino disappearance from atmospheric neutrino...Go to contribution page
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Prof. Mark Vagins (Kavli IPMU)20/07/2014, 14:10WATCHMAN is a US project designed to demonstrate the feasibility of using a large gadolinium-loaded water Cherenkov detector to remotely locate clandestine nuclear reactors in uncooperative nations via their antineutrino emissions. The current status and upcoming plans for WATCHMAN in its nonproliferation role will be discussed, as well as its expected physics output.Go to contribution page
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Dr Taku Ishida (KEK)20/07/2014, 14:40Recent operational status of the accelerators at J-PARC will be reviewed, and necessary steps towards achieving the design 750 kW beam power, and further ideas to realize MW-class beam operation, will be presented.Go to contribution page
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Dr Tetsuro Sekiguchi (KEK)20/07/2014, 15:00The J-PARC neutrino beamline has had beam operation in the period May-June 2014 after a year long shutdown. Several beamline components were upgraded during the shutdown. The main upgrade was a replacement of all three magnetic horns. The new magnetic horns were upgraded to improve the acceptable beam power and to solve some known problems. The operation status of the neutrino beamline will be...Go to contribution page
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Dr Yuichi Oyama (KEK)20/07/2014, 15:20Upgrade plan of the neutrino beam-line for multi-MW beam in coming several years is reported.Go to contribution page
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Dr Daniel Winklehner (MIT)20/07/2014, 15:40The proposed Decay-At-rest Experiment for δCP violation At the Laboratory for Underground Science (DAEδALUS) and the Isotope Decay-At-Rest experiment (IsoDAR), search for CP violation in the neutrino sector and sterile (non-interacting) neutrinos. Both are short baseline experiments that use proton driver beams. In the IsoDAR case, a 60 MeV proton beam will impinge on a high purity...Go to contribution page
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Prof. Francesca Di Lodovico (Queen Mary, University of London)20/07/2014, 16:10In this talk we will first describe the current computing infrastructure, ie the software release structure, how to access the code, the efforts to get an independent Hyper-K software code, etc. Then, we will describe the current status of the MC physics production with the latest release and how to access the simulated data.Go to contribution page
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Prof. Tsuyoshi NAKAYA (Kyoto)20/07/2014, 16:30
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Prof. Masashi Yokoyama (University of Tokyo)21/07/2014, 09:00
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Ms Linda Cremonesi (Queen Mary University of London)21/07/2014, 09:10We will present the sensitivity studies for the Hyper-Kamiokande experiment assuming 7.5MW total integrated POT and 320 kA horn current. The systematic errors from a few different sources have been included: near detector (ND280) fit constrained parameters, parameters non-constrained by the near detector fit, Hyper-K detector systematics (rescaled from the Super-K one) and FSI parameters. We...Go to contribution page
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Mr raj shah (oxford university)21/07/2014, 09:30We will present sensitivity studies for T2HK assuming a total integrated beam power of 7.5MW years and a 320kA horn current. The studies presented will focus on the effect and limitations caused by the current sources of systematic errors for T2K.Go to contribution page
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Dr Yusuke Koshio (Okayama university)21/07/2014, 09:40The modified sensitivity for the solar neutrino in Hyper-Kamiokande using the correct depth will be reported.Go to contribution page
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Dr Hide-Kazu TANAKA (ICRR, University of Tokyo)21/07/2014, 10:15I will discuss Hyper-K candidate site and cavern construction.Go to contribution page
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Dr Shoei Nakayama (Kamioka Observatory, ICRR, University of Tokyo)21/07/2014, 10:45This talk will discuss current status and plan of Hyper-K tank design, and also cover status of technical design document for the tank design.Go to contribution page
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Dr Hiroyuki Sekiya (ICRR/IPMU)21/07/2014, 11:15Topics of the talk are as follows; 1. The updated water purification system based on vacuum degasifiers instead of membrane degasifiers. 2. The results of the simulation of the water flow in the tank.Go to contribution page
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Prof. Mark Vagins (IPMU)21/07/2014, 11:30The current status of and plans for EGADS, the main Gd test facility for Super-K and Hyper-K, will be discussed.Go to contribution page
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Dr Shoei Nakayama (Kamioka Observatory, ICRR, University of Tokyo)21/07/2014, 12:40I will present a brief introduction of current activities in the photodetector sub-WG and the plan for the photodetector development.Go to contribution page
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Mr Yuji Okajima (Tokyo Institute of Technology)21/07/2014, 12:50In August 2013, eight hybrid photodetectors (HPDs) with 20-cm diameter and five 50-cm High-QE (HQE) photomultiplier tubes (PMTs) have been installed into a water tank and a validity test started. I will present a progress and results on the 20-cm HPDs and 50-cm HQE PMTs test in the water tank and a status and plan for a next test with new 50-cm box-and-line dynode PMTs.Go to contribution page
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Mr Yusuke Suda (University of Tokyo)21/07/2014, 13:10We have been developing 50-cm diameter Box&line PMTs and Hybrid Photo-Detectors (HPDs) for Hyper-Kamiokande. Both have excellent performance compared with Super-Kamiokande PMT. We present the principle and basic performance (typical waveforms, timing response, dark count rate, linearity and response uniformity) and the result of the pre-calibration for a test in a 200-ton water Cherenkov...Go to contribution page
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Dr Yasuhiro NISHIMURA (ICRR)21/07/2014, 13:30The R&D of photosensors and plan in Kamioka, Japan, are presented.Go to contribution page
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Dr Yoshinari Hayato (Kamioka obs., ICRR, Univ. of Tokyo)21/07/2014, 13:50
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Mr Perry Sandstrom (WIPAC)21/07/2014, 14:05This talk will present the status of the next generation digital optical module being designed for the IceCube upgrade detectors.Go to contribution page
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Dr Helen O'Keeffe (Lancaster University)21/07/2014, 14:20Within the UK, several institutions will participate in the development of Data Acquisition systems (DAQ) for the Hyper-Kamiokande experiment. This talk will discuss UK interests, physics considerations for the design of the DAQ and progress towards a conceptual design.Go to contribution page
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Dr Fabrice Retiere (Triumf)21/07/2014, 14:35
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Dr Makoto Miura (Kamioka Observatory, ICRR, University of Tokyo)21/07/2014, 15:10This is a introduction talk for the software session. It shows what are going to be discussed in the session.Go to contribution page
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Mr Yuji Okajima (Tokyo Institute of Technology)21/07/2014, 15:20Baseline design of the Hyper-Kamiokande detector has been implemented in WCSim, a simulation software developed to study the detector design and physics potential of HK. In addition, implementation of new photo sensors and other detailed detector components are ongoing to evaluate the impact on the performance of the HK detector, including the energy resolution and particle identification. In...Go to contribution page
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Dr Takatomi Yano (Okayama Univ.)21/07/2014, 15:50Bonsai is a reconstruction algorithm for low energy events at Super-K. Here, R&D of bonsai with WCsim and application for Hyper-K will be reported.Go to contribution page
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Prof. Blair Jamieson (University of Winnipeg), Dr Michael Wilking (TRIUMF)21/07/2014, 16:02The current status of the fiTQun event reconstruction for Hyper-Kamiokande events will be presented.Go to contribution page
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Dr Makoto Miura (Kamioka Observatory, ICRR, University of Tokyo)21/07/2014, 16:27I will summarize developments of software towards Hyper-K and show some prospects.Go to contribution page
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Dr Hide-Kazu TANAKA (ICRR, University of Tokyo)21/07/2014, 17:00I will discuss overview of HK calibration R&D and prototyping projects.Go to contribution page
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Dr Neil McCauley (University of Liverpool)21/07/2014, 17:05LED pulsers can provide nanosecond scale pulses ideal for the calibration of Hyper-Kamiokande. The latest developments in the design of a prototype driver for Hyper-Kamiokande in the UK will be presented.Go to contribution page
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Dr Takatomi Yano (Kobe Univ.)21/07/2014, 17:20Because of the large detector, Hyper-K will need an automated calibration source deployment system. Here, the status of R&D of automated calibration source deployment system will be reported.Go to contribution page
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Dr Tom Feusels (University of British Columbia)21/07/2014, 17:35I will discuss the status of the Photosensor Testing Facility (PTF) which is currently being built at TRIUMF. The PTF will measure the optical properties (acceptance, reflectivity, ...) of the PMTs under investigation for Hyper-Kamiokande using two robotic gantries.Go to contribution page
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Dr Szymon Manecki (Queen's University)21/07/2014, 17:50SNO+ is a 780-ton liquid scintillator detector that aims at measuring neutrinoless double beta decay of Te-130 using the underground facility at SNOLAB and the original SNO detector. In this talk, the SNO+ detector design and calibration hardware will be presented with an overview of the new physics goals and potential.Go to contribution page
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Prof. Mark Hartz (Kavli IPMU (WPI), The University of Tokyo/TRIUMF)22/07/2014, 09:00
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Dr Minfang Yeh (Brookhaven National Laboratory)22/07/2014, 09:05The newly developed, water-based liquid scintillator (WbLS) is an advanced scintillation liquid for future massive detectors with the unique capability of exploring physics below the Cherenkov threshold and has the ability of loading any (hydrophilic) metallic ions of interest for neutron tagging or other physics enhancements. The same water-based detector could also be used as a near...Go to contribution page
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Prof. Mark Hartz (Kavli IPMU (WPI), The University of Tokyo/TRIUMF)22/07/2014, 09:30The sensitivities for measuring CP violation and other neutrino oscillation parameters in a Tokai-to-Hyper-K long baseline experiment depend on systematic uncertainties in the neutrino flux and cross section models. These model uncertainties are constrained by data from near detectors. In this talk, I will present studies of the effect of near detector data on the CP violation sensitivity...Go to contribution page
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Dr David Hadley (University of Warwick)22/07/2014, 09:45The TITUS detector is an original multi-purpose new detector for the Hyper-K experiment, located 2 km from the J-PARC neutrino beam. TITUS consists of a gadolinium-doped water Cherenkov detector, partially enclosed by a muon range detector (MRD) The detector will be exposed to a neutrino flux similar to the Hyper-K far detector, minimising the uncertainty on the near-to-far extrapolation. The...Go to contribution page
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Dr Mark Rayner (Université de Genève)22/07/2014, 10:05This talk will describe the advantages of surrounding the proposed 2km TITUS water Cherenkov with a magnetized iron range detector. The benefits for sample size, energy resolution and charge reconstruction will be discussed.Go to contribution page
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Dr Michael Wilking (TRIUMF)22/07/2014, 10:25In order to reach the projected T2HK physics sensitivities, a better understanding of neutrino interaction uncertainties is required. The nuPRISM detector concept is a novel new technique to directly measure neutrino interaction final states for any oscillated spectra at Hyper-K. This removes neutrino interaction uncertainties from the accelerator-based oscillation measurements, and provides...Go to contribution page
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Dr Mark Scott (TRIUMF)22/07/2014, 10:45The nuPRISM detector concept provides a powerful tool for neutrino physics, using measurements at multiple off-axis angles to produce oscillated or mono-energetic neutrino beams. This talk describes the current long baseline sensitivity studies with nuPRISM, quantitatively demonstrating the benefits this technique brings to oscillation analyses. It will also discuss the short baseline...Go to contribution page
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22/07/2014, 11:40
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Dr Morgan Wascko (Imperial College London)One of the dominant sources of systematic uncertainty in the HK CPV search will stem from neutrino-nucleus interaction modelling. Gas TPC detectors, which have fine-grained final-state particle reconstruction, excellent particle identification, low particle momentum thresholds, and the ability to change target nucleus, provide a unique opportunity for neutrino-nucleus interaction-model...Go to contribution page
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Mr Benjamin Quilain (Ecole Polytechnique, Laboratoire Leprince-Ringuet, In2p3)The Lorentz invariance violation (LV) arises at Planck scale, as a consequence of merging standard model and gravity. Though LV effects are naturally highly supressed at low energy, possible measurable effects are predicted in sensitive channels as neutrino oscillations. In this channel, LV operates both by modifying the PMNS oscillations at far detector, but also predicting new oscillations...Go to contribution page
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Prof. Darren Grant
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Dr Dawn WilliamsRecent updates from the design studies of the PINGU project will be presented.Go to contribution page
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