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International Workshop on Next Generation Nucleon Decay and Neutrino Detectors (NNN18)

October 31, 2018 to November 4, 2018
UBC Robson Square
America/Vancouver timezone

Contribution List

101 out of 101 displayed
  1. 99. Introduction: Status of HyperK and opportunities
    Prof. Masato SHIOZAWA (Kamioka Observatory, ICRR, The University of Tokyo)
    2018-10-31, 2:00 p.m.
  2. 100. Physics with higher energy neutrinos at HyperK
    Dr Akira Konaka (TRIUMF)
    2018-10-31, 2:45 p.m.
  3. 101. Neutrino astrophysics at HyperK
    Dr Michael Smy (University of California, Irvine)
    2018-10-31, 3:30 p.m.
  4. 102. HyperK detector
    Shoei Nakayama (Kamioka Observatory, ICRR, University of Tokyo)
    2018-10-31, 4:15 p.m.
  5. 105. Analysis and Systematics
    Dr Mark Hartz (Kavli IPMU (WPI), University of Tokyo/TRIUMF)
    2018-10-31, 5:00 p.m.
  6. 1. Welcome
    Dr Jonathan Bagger (TRIUMF)
    2018-11-01, 8:00 a.m.
  7. 2. Experimental Overview of Neutrino Oscillations
    Prof. Mark Messier (Indiana)
    2018-11-01, 8:10 a.m.
  8. 3. Origin of Neutrino mass
    Prof. Shun Zhou (IHEP)
    2018-11-01, 8:40 a.m.
  9. 4. Theoretical overview of neutrino oscillation
    Mr Carlo Giunti (INFN)
    2018-11-01, 9:00 a.m.
  10. 5. Neutrinos and muti-messenger signatures for a galactic supernova
    Prof. Kei Kotake (Fukukoka)
    2018-11-01, 9:20 a.m.
  11. 6. New development of the underground facilities
    Shoei Nakayama (Kamioka Observatory, ICRR, University of Tokyo)
    2018-11-01, 9:40 a.m.
  12. 7. T2K
    Dr Laura Kormos (Lancaster University)
    2018-11-01, 10:30 a.m.
  13. 8. NOvA
    Gregory Pawloski (University of Minnesota)
    2018-11-01, 10:55 a.m.
  14. 9. IceCube
    Dr Joanna Kiryluk (Stonybrook)
    2018-11-01, 11:20 a.m.
  15. 10. SuperK (Atmospheic, proton decays)
    Dr Shunichi Mine (University of California, Irvine)
    2018-11-01, 11:45 a.m.
  16. 11. Poster talks (1)
    Ms Jashanjot Kaur Brar (University of Winnipeg), Prof. Jianming Bian (UC Irvine), Dr Karin Gilje (University of Alberta), Micah Buuck (University of Washington - Seattle), Dr Vincent Fischer (University of California at Davis), Dr Yang Zhang (University of Alberta)
    2018-11-01, 12:10 p.m.
    Poster talks Thu, Nov 1: - Update on the $hep$ solar neutrino limit from the three-phase SNO dataset - GILJE, Karin - Neutron detection in the water phase of SNO+ experiment - ZHANG, Yang - LEGEND: The Large Enriched Germanium Experiment for Neutrinoless Double-Beta Decay - BUUCK, Micah - Energy Reconstruction in NOvA with Regression Convolutional Neural Networks - BIAN, Jianming -...
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  17. 82. Deep Learning Techniques Overview
    Dr Terao Kazuhiro (SLAC National Accelerator Laborator)
    2018-11-01, 2:00 p.m.
  18. 66. The IceCube Neutrino Observatory: Detector Status and Designs for the Future
    John Kelley (University of Madison–Wisconsin)
    2018-11-01, 2:00 p.m.
    parallel talk
    Detector parallel
    The IceCube Neutrino Observatory is a cubic-kilometer-scale neutrino detector and cosmic ray air shower array at the geographic South Pole. The detector consists of over 5400 digital optical modules (DOMs), with 98.5% of modules still taking data. High detector uptime and a real-time Iridium satellite link have helped to facilitate recent astrophysical neutrino discoveries. Prototype air...
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  19. 53. STRAW – STRings for Absorption length in Water
    Dr Christian Fruck (Technical University Munich (TUM))
    2018-11-01, 2:20 p.m.
    parallel talk
    Detector parallel
    Recent results presented by IceCube have demonstrated the potential of large instrumented volume type detectors for multi-messenger astronomy using neutrinos. Conducting deep astronomical observations with such type of detector requires increasing the sensitivity and therefore mostly the detector volume by around 2 orders of magnitude, a goal that might not be achievable with a single...
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  20. 77. Machine Learning Techniques on NOvA
    Dr Micah Groh (Indiana University)
    2018-11-01, 2:30 p.m.
    The NOvA experiment has made measurements of the disappearance of νµ and the appearance of νe in the NuMI beam at Fermilab including the neutrino mass hierarchy and the CP violating phase. Key to these measurements is the application of machine learning methods for identification of neutrino flavor and energy reconstruction. These methods require rigorous validation to both understand and...
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  21. 88. Liquid Scintillator development
    Minfang Yeh (Brookhaven National Lab)
    2018-11-01, 2:40 p.m.
  22. 83. Machine Learning at MINERvA
    Dr Anushree Ghosh (Universidad Técnica Federico Santa María)
    2018-11-01, 2:50 p.m.
  23. 50. Spectral Sorting of Photons Using Dichroic Winston Cones
    Mr Tanner Kaptanoglu (University of Pennsylvania)
    2018-11-01, 3:00 p.m.
    parallel talk
    Detector parallel
    Large-scale neutrino detectors typically observe photons created by interactions inside of the target volume. These detectors deploy a wide variety of technologies, most commonly water, ice, or scintillator targets surrounded by PMTs. The detected photons carry information that goes unused, most notably the wavelength, which can indicate the production method and travel time of the photon. In...
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  24. 84. Machine Learning in MicroBooNE
    Prof. Taritree Wongjirad (Tufts University)
    2018-11-01, 3:10 p.m.
  25. 44. The MCP-PMT for Neutrino Detector
    Dr Sen QIAN (IHEP,CAS)
    2018-11-01, 3:15 p.m.
    parallel talk
    Detector parallel
    Microchannel plate (MCP) is always used in the small PMTs as the electron multiplier for the fast timing detection, which greatly improved the time resolution of PMT. The large scaler neutrino detectors, such as SuperK, DayaBay, JUNO and HyperK, need the large area PMTs for the large photocathode coverage and less electronic channels. Usually there was only one type of 20 inch PMT based on the...
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  26. 58. Systematics, calibration and analysis techniques in JUNO
    Prof. Jian Tang (Sun Yat-Sen University)
    2018-11-01, 3:55 p.m.
    The Jiangmen Underground Neutrino Observatory(JUNO) is a liquid scintillator detector aiming to determine the neutrino mass hierarchy and to perform precision measurements of neutrino mixing parameters by detecting reactor antineutrinos at a baseline of 53 km. JUNO physics programme also serves for the detection of supernova neutrinos, geoneutrinos and solar neutrinos. In order to achieve the...
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  27. 89. Review of photo-detectors for huge detectors
    Prof. Liangjian Wen (Institute of High Energy Physics, Chinese Academy of Sciences)
    2018-11-01, 4:00 p.m.
  28. 90. Large Area Picosecond Photo-detectors
    Alexey Lyashenko (Incom Inc)
    2018-11-01, 4:20 p.m.
  29. 86. Systematic errors in Borexino Solar and Geoneutrino Analyses
    Prof. Livia Ludhova Ludhova (Forschungszentrum Juelich)
    2018-11-01, 4:20 p.m.
    Borexino is the world radio-purest large-volume liquid-scintillator detector placed at the Laboratori Nazionali del Gran Sasso in Italy. Since the start of its data taking in May 2007, it has provided several measurements of solar neutrinos and geoneutrinos. Recently, Borexino has released new results concerning comprehensive spectroscopy of the pp-chain solar neutrinos. The talk will brifely...
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  30. 91. 20" PMT development for Hyper-K
    Jun Kameda (University of Tokyo)
    2018-11-01, 4:40 p.m.
  31. 85. Systematic Uncertainties for Atmospheric Neutrino Measurements
    Prof. Juan Pablo Yañez (University of Alberta)
    2018-11-01, 4:45 p.m.
  32. 92. Electronics for E61 multi-PMTs
    Dr Thomas Lindner (TRIUMF)
    2018-11-01, 4:55 p.m.
    We propose using multi-PMTs (mPMTs) for the photosensors for the E61 near detector (as well as a fraction of Hyper-K photosensors). Our mPMT design has nineteen 3" PMTs enclosed in water-tight pressure vessel, providing excellent spatial imaging of the Cherenkov light ring. This talk will describe the design of the signal digitization electronics for the E61 mPMTs. We will start by explaining...
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  33. 80. Test Beam Experiments for the Future Generation of LBL Experiments
    Stefania Bordoni (CERN)
    2018-11-01, 5:10 p.m.
    The next generation of LBL experiments is currently under preparation. These future experiments will profit from new and high intensity neutrino beams which will allow very large samples of data to be collected. A deep understanding and strong constraint of the systematic uncertainties is thus mandatory to achieve precision measurements and to allow the experiments to fulfil their physics...
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  34. 93. The T2K ND280 upgrade project
    Etam Noah (University of Geneva)
    2018-11-01, 5:10 p.m.
  35. 65. Update on the $hep$ solar neutrino limit from the three-phase SNO dataset
    Dr Karin Gilje (University of Alberta)
    2018-11-01, 6:00 p.m.
    The spectrum of solar neutrinos from the $pp$ chain has been studied in depth by a variety of underground detectors. However, neutrinos from the $hep$ reaction (${}^3$He $+$ $p^+$ $\rightarrow$ ${}^4$He $+$ $e^+$ + $\nu_e$) remain unobserved due to the small theoretical branching ratio ($2\times10^{−7}$ per $pp$ termination). The SNO detector has a unique sensitivity to neutrino energies...
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  36. 52. Neutron detection in the water phase of SNO+ experiment
    Dr Yang Zhang (University of Alberta)
    2018-11-01, 6:03 p.m.
    Efficient detection of neutrons in water is important because of its physics applications. For example, neutron detection could enable the detection of neutrinos via inverse beta decay or help suppress neutron-accompanied backgrounds. However, observing neutrons in pure water Cherenkov detectors is a challenging task due to the low energy of the 2.2 MeV gamma emitted upon capture. SNO+ is a...
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  37. 70. LEGEND: The Large Enriched Germanium Experiment for Neutrinoless Double-Beta Decay
    Micah Buuck (University of Washington - Seattle)
    2018-11-01, 6:06 p.m.
    The lepton number violating process of neutrinoless double-beta decay could result from the physics beyond the Standard Model needed to generate the neutrino masses. Taking different approaches, the current generation of ${}^{76}$Ge experiments, the MAJORANA DEMONSTRATOR and GERDA, lead the field in both the ultra-low background and energy resolution achieved. The next generation of...
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  38. 49. Energy Reconstruction in NOvA with Regression Convolutional Neural Networks
    Prof. Jianming Bian (UC Irvine)
    2018-11-01, 6:09 p.m.
    NOvA is a long-baseline accelerator 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. NOvA aims to resolve the mass hierarchy, the CP violation and the octant of theta23. We will focus on the development and application of deep learning to the...
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  39. 72. R&D on Water-based Liquid Scintillator for the Theia experiment
    Dr Vincent Fischer Fischer (University of California at Davis)
    2018-11-01, 6:12 p.m.
    Recent developments in the field of liquid scintillator chemistry and fast-timing photosensors paved the way for a new generation of large-scale detectors, such as Theia, capable of tackling a broad range of physics issues. Water-based Liquid Scintillator (WbLS) is a novel detection medium that combines the advantages of pure water, including low attenuation, accurate direction reconstruction,...
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  40. 68. HALO-1kt: A massive helium and lead observatory for supernova neutrinos
    Dr Matthew Geske (Gonzaga University)
    2018-11-01, 6:18 p.m.
    HALO-1kt is a supernova neutrino observatory which would leverage 1000 tonnes of lead from the decommissioned OPERA experiment to create a low cost and low maintenance neutrino detector. It is to be sited at LNGS, and is intended to operate as a scaled up version of the original HALO. Due to its sensitivity to $\nu_e$, it is complementary to water Cherenkov and liquid scintillator-based...
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  41. 63. Model-independent reconstruction of full flavor supernova neutrino spectra in future large liquid-scintillitor detectors
    Dr Huiling Li (Institute of High Energy Physics)
    2018-11-01, 6:21 p.m.
    The fortunate observation of neutrino events from the SN1987A explosion in the Large Magellanic Cloud is a milestone in both neutrino physics and neutrino astronomy. The sparse data, however, can't provide us the accurate energy spectra of supernova neutrinos. Currently many worldwide neutrino detectors runnning or under construction have better detection capbilities of core collapse...
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  42. 54. Search for Supernova Neutrinos with the LVD Experiment
    Dr CARLO FRANCESCO VIGORITO (UNIVERSITY and INFN , Torino, Italia)
    2018-11-01, 6:24 p.m.
    The Large Volume Detector (LVD) is continuously taking data since 1992 at the INFN Gran Sasso National Laboratory (Italy). The experiment, 1 kton of liquid scintillator organized in 840 counters, is sensitive in the neutrino channels to burst expected from a gravitational stellar collapse. Full detection probability is foreseen in the case of an unexpected event in the Milky Way, d<25 kpc....
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  43. 62. The Central Detector of JUNO
    Mr Yatian Pei (The Institute of High Energy Physics (IHEP))
    2018-11-01, 6:27 p.m.
    Jiangmen Underground Neutrino Observatory (JUNO) is an experiment under construction in Southern China. It aims to determine the neutrino mass hierarchy, to measure precisely the oscillation parameters by detecting reactor neutrinos from nuclear power plants, to observe supernova neutrinos, to study the atmospheric, solar neutrinos and geo-neutrinos, and to perform exotic searches. As the...
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  44. 57. Detection of electron anti-neutrino at Jinping
    Mr Jinjing Li (Tsinghua University)
    2018-11-01, 6:33 p.m.
    The China Jinping Underground Laboratory (CJPL) with the lowest cosmic-ray muon flux and the lowest reactor neutrino flux of any laboratory is ideal to carry out low-energy neutrino experiments for solar neutrino, geo-neutrino and supernova neutrino physics studies. At present, a 1-ton prototype for Jinping Neutrino Experiment of which the target material is liquid scintillator is deployed in...
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  45. 12. SK and SK-Gd (solar and supernova)
    Dr Michael Smy (University of California, Irvine)
    2018-11-02, 9:00 a.m.
  46. 13. Daya Bay/Reno/Double Chooz
    Prof. Henry Band (Yale)
    2018-11-02, 9:20 a.m.
  47. 14. SNO+
    Dr Morgan Askins (UC Berkeley)
    2018-11-02, 9:45 a.m.
  48. 15. Review of Double Beta Decay Experiments
    Dr Azusa Gando (RCNS, Tohoku University)
    2018-11-02, 10:05 a.m.
  49. 16. HyperK
    Dr Adrian Pritchard (University of Liverpool)
    2018-11-02, 11:00 a.m.
  50. 17. DUNE
    Prof. Alexandre Sousa (Cinsinnati)
    2018-11-02, 11:25 a.m.
  51. 18. JUNO
    Prof. Alberto Garfagnini (INFN Padova)
    2018-11-02, 11:50 a.m.
  52. 19. Poster talks (2)
    Dr CARLO FRANCESCO VIGORITO (UNIVERSITY &amp; INFN , Torino, Italia), Dr Huiling Li (Institute of High Energy Physics), Mr Jinjing Li (Tsinghua University), Dr Matthew Geske (Gonzaga University), Mr Yatian Pei (The Institute of High Energy Physics (IHEP))
    2018-11-02, 12:15 p.m.
    Poster talks Fri, Nov 2: - HALO-1kt: A massive helium and lead observatory for supernova neutrinos - GESKE, Matthew - Model-independent reconstruction of full flavor supernova neutrino spectra in future large liquid-scintillitor detectors - LI, Huiling - Search for Supernova Neutrinos with the LVD Experiment - VIGORITO, Carlo Francesco - The Central Detector of JUNO - PEI, Yatian -...
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  53. 81. Neutrino Interaction Uncertainties in Long Baseline Oscillation Experiments
    Dr Chris Marshall (Lawrence Berkeley National Laboratory)
    2018-11-02, 2:00 p.m.
    Uncertainties on neutrino-nucleus scattering cross sections are among the dominant systematics in long-baseline neutrino oscillation experiments, despite partial cancellation from near detector measurements. I will review the most important issues facing current experiments, and discuss what is required for next generation precision measurements.
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  54. 69. The Astroparticle and Exotic Physics program of MicroBooNE
    Dr Crespo-Anadón José I. (Columbia University Nevis Laboratories)
    2018-11-02, 2:00 p.m.
    parallel talk
    Detector parallel
    MicroBooNE is a liquid argon time projection chamber (LArTPC) with an 85-ton active mass situated on the Booster Neutrino Beam at Fermilab. Some of the experiment goals are investigating the excess of electron-like events observed in MiniBooNE, performing cross-section measurements of neutrino interactions in argon and gaining knowledge about the operation and the detector physics of LArTPCs...
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  55. 55. Sterile neutrino searches with the ICARUS detector
    Dr Hannah Rogers (Colorado State University)
    2018-11-02, 2:20 p.m.
    parallel talk
    Detector parallel
    The 760 ton ICARUS T600 detector performed a successful three-year physics run at the underground LNGS laboratories studying neutrino oscillations with the CNGS neutrino beam from CERN, and searching for atmospheric neutrino interactions. ICARUS performed a sensitive search for LSND like anomalous $\nu_e$ appearance in the CNGS beam, which contributed to constrain the allowed parameters...
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  56. 78. DUNE Analysis Methods and Systematic Uncertainties
    Dr Christopher Backhouse (University College London)
    2018-11-02, 2:30 p.m.
    The twin challenges facing the DUNE long-baseline analysis are to extract the maximum statistical power from the Far Detector data while minimizing the impact of systematic uncertainties. The liquid argon TPCs that make up the DUNE Far Detector will provide outstanding spatial resolution, and should allow neutrino flavours to be separated with high efficiency and purity. However, taking...
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  57. 74. ProtoDUNE SP R&D
    Ms Francesca Stocker (CERN)
    2018-11-02, 2:40 p.m.
    parallel talk
    Detector parallel
    ProtoDUNE-SP is the single-phase DUNE Far Detector prototype that was recently built at CERN and is in operation since September 2018. ProtoDUNE-SP is a crucial part of the DUNE effort towards the construction of the first DUNE 10-kt fiducial mass far detector module (17 kt total LAr mass), but also a significant experiment in its own right. With a total liquid argon (LAr) mass of 0.77 kt, it...
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  58. 71. Systematics in Hyper-Kamiokande experiment
    Tomoyo Yoshida (Tokyo Institute of Technology)
    2018-11-02, 2:55 p.m.
    Hyper-Kamiokande is a next-generation underground water-Cherenkov detector, which is to be constructed from 2020. The physics program of Hyper-K includes a nucleon-decay search, a CP-phase measurement in the lepton sector with an accelerator neutrino beam, the determination of the neutrino mass hierarchy with atmospheric neutrinos, and the observation of astrophysical neutrinos. Thanks to...
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  59. 94. ArgonCube: LArTPC R&D for the DUNE Near Detector
    James Sinclair (U. Bern)
    2018-11-02, 3:00 p.m.
  60. 95. R&D on pixel readout for DUNE near detector
    Dan Dwyer (LBNL)
    2018-11-02, 3:15 p.m.
  61. 73. Analysis and Systematic Uncertainty Experience from MicroBooNE
    Mr Salvatore Davide Porzio (The University of Manchester)
    2018-11-02, 3:20 p.m.
    The MicroBooNE detector is a Liquid Argon Time Projection Chamber (LArTPC) with an 85-ton active mass, situated at Fermilab in the Booster Neutrino Beam and designed to study short-baseline neutrino physics. Its main physics goals include the investigation of the anomalous excess of electron-like events observed in MiniBooNE, the measurement of low-energy, neutrino-argon cross-sections and the...
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  62. 67. DUNE electronics, trigger and DAQ
    Dr Babak Abi (University of Oxford)
    2018-11-02, 4:00 p.m.
    parallel talk
    Detector parallel
    Deep Underground Neutrino Experiment (DUNE), which is consist of two neutrino detectors placed near and far of Fermilab, will address several questions in neutrino physics. In addition, It intends to facilitate the study of neutrinos from the supernova and search for proton decay. The liquid argon time projection chamber (LArTPC) technology has been adopted to detect the neutrino...
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  63. 75. Uncertainties from Neutrino Interactions at T2K
    Kevin McFarland (University of Rochester)
    2018-11-02, 4:10 p.m.
    The oscillation analysis at T2K, even with limited statistics, has needed to improve and constrain the model of neutrino interactions in order to reach its current sensitivity. I review the interaction model, some of the most important uncertainties in the model for the oscillation analysis, and techniques for constraining those uncertainties through measurements of neutrino interactions.
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  64. 96. DUNE signal processing
    Dr Hannah Rogers (Colorado State University)
    2018-11-02, 4:20 p.m.
  65. 79. Details of Systematic Uncertainties at NOvA
    Dr Louise Suter (Fermi National Accelerator Laboratory)
    2018-11-02, 4:35 p.m.
    I will present the details of the systematic uncertainties at NOvA for the latest measurements of both (anti)neutrino electron appearance and muon disappearance, as well as the systematic uncertainties associated with recent cross section results. NOvA is a long-baseline neutrino experiment which utilizes two basically fully active, finely segmented, liquid scintillator detectors: a Near...
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  66. 56. First Results From ARIADNE: A 1-ton dual-phase LArTPC with optical readout.
    Mr Adam Roberts (University of Liverpool), Dr Kostas Mavrokoridis (University of Liverpool)
    2018-11-02, 4:40 p.m.
    parallel talk
    Detector parallel
    ARIADNE is a 1-ton two-phase liquid argon (LAr) time projection chamber (TPC) featuring a novel optical readout method. The detector uses a Thick Gas Electron Multiplier (THGEM) in the extraction region to generate secondary scintillation light which is imaged using 4 Electron-Multiplying (EM)CCD cameras to produce high resolution images of particle interactions within the detector. This...
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  67. 76. Interaction Modeling Uncertainties at MINERvA
    Kevin McFarland (University of Rochester)
    2018-11-02, 5:00 p.m.
    MINERvA began its cross section measurement program with a default model that looks very different than the used in its most recent measurement. I summarize the improvements and the measurements that have driven those changes. Recent data highlights areas in need of future refinement. I also discuss how the results of these improvements may be utilized by other experiments for their modeling.
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  68. 97. Light detection in DUNE
    Zelimir Djurcic (Argonne National Lab)
    2018-11-02, 5:00 p.m.
  69. 20. Systematic Uncertainty in Future Neutrino Oscillation Experiments
    Prof. Michael Wilking (Stony Brook University)
    2018-11-03, 9:00 a.m.
  70. 21. HyperK Near Detectors
    Dr John Walker (Winnipeg)
    2018-11-03, 9:25 a.m.
  71. 22. DUNE Near Detectors
    Dr Chris Marshall (LBNL)
    2018-11-03, 9:45 a.m.
  72. 23. Short Baseline Neutirno Experiments
    Brooke Russell (Yale University)
    2018-11-03, 10:05 a.m.
  73. 24. Ultra-high energy neutrinos
    Prof. Nathan Whitehorn (UCLA)
    2018-11-03, 11:00 a.m.
  74. 25. KM3NeT
    Christine Nielsen (APC)
    2018-11-03, 11:25 a.m.
  75. 26. IceCube Gen2
    Dr Joshua Hignight (Alberta)
    2018-11-03, 11:45 a.m.
  76. 27. WATCHMAN
    Prof. Christopher Mauger (University of Pennsylvania)
    2018-11-03, 12:05 p.m.
  77. 29. Solar and Supernova neutrinos (present and future)
    Erin O'Sullivan (Stockholm University)
    2018-11-03, 2:00 p.m.
  78. 31. Jingping
    Prof. Jian Tang (Sun Yat-Sen University)
    2018-11-03, 2:25 p.m.
  79. 32. THEIA
    Prof. Gabriel Orebi Gann (UC Berkeley / LBNL)
    2018-11-03, 2:45 p.m.
  80. 30. ANNIE
    Dr Vincent Fischer Fischer (University of California at Davis)
    2018-11-03, 3:05 p.m.
  81. 33. Summary of the Detector Parallel session
    Dr Fabrice Retiere (TRIUMF)
    2018-11-03, 4:00 p.m.
  82. 34. Summary of the systematics and analysis technique parallel
    Dr Mark Hartz (Kavli IPMU (WPI), University of Tokyo/TRIUMF)
    2018-11-03, 4:25 p.m.
  83. 35. Workshop summary
    Prof. Masayuki Nakahata (ICRR Tokyo)
    2018-11-03, 4:50 p.m.
  84. 37. Report from the steering committee
    Prof. Chang Kee Jung (Stonybrook)
    2018-11-03, 5:15 p.m.
  85. 38. Next NNN
    Prof. David Martinez Caicedo (South Dakota School of Mines and Technology), Prof. David Martinez Caicedo (South Dakota School of Mines and Technology)
    2018-11-03, 5:25 p.m.
  86. 39. End of the workshop
    2018-11-03, 5:35 p.m.
  87. 103. HyperK analysis and systematics
    Dr Mark Hartz (TRIUMF/IPMU)
  88. 64. IceCUBE detector system
    John Kelley (University of Wisconsin)
  89. 43. Low-energy neutrino detection with Borexino
    Prof. Livia Ludhova (Forschungszentrum Juelich)
    parallel talk
    Borexino is the world radio-purest large-volume liquid-scintillator detector placed at the Laboratori Nazionali del Gran Sasso in Italy. Since the start of its data taking in May 2007, it has provided several measurements of solar neutrinos, important for the understanding of our star, as well as of the neutrino properties. In particular, Borexino has performed the first spectroscopic...
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  90. 28. Poster talks (3)
  91. 59. Preliminary design study for Jinping neutrino experiment
    Mr Wentai Luo (University of Chinese Academy of Sciences)
    poster
    Jinping underground neutrino experiment kton-detector will be built in the future. We use the simulation software — Jinping Simulation Analysis Package(JSAP) based on Geant4 for simulating and optimizing the kton-detector structure. Each part of the detector is likely to have uranium, thorium, potassium or radon radioactive isotopes, which will be our background. Based on some simulations, we...
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  92. 36. Report on IUPAP Neutrino panel
    Dr Nigel Smith (SNOlab)
  93. 60. Review of Double Beta Decay Experiments
    Dr Azusa Gando (RCNS, Tohoku University)
    Neutrinoless double beta (0nbb) decay violates lepton number conservation and it requires two characteristic neutrino properties; non-zero mass and Majorana nature of the neutrino. Assuming the minimal mechanism of the decay, it would constrain the neutrino mass hierarchy and mass scale. In nature, more than 60 of isotopes are known as double beta decay nuclei, however, there is no perfect...
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  94. 87. Review of Short Baseline Neutrino Experiments
    Brooke Russell (Yale University)
    In this talk, I will review the present landscape in short baseline neutrino experiments as it relates to sterile neutrino physics. After describing recent results from short baseline reactor and accelerator experiments, I will focus on recent results from the MicroBooNE experiment, as it systematically builds towards a definitive test of the MiniBooNE low energy excess. In addition, I will...
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  95. 61. SoLid: Latest results and futures plans
    Dr Behzad Hosseini (Imperial College London)
    poster
    The SoLid experiment is a short-baseline (6-9 m) nuclear reactor experiment that targets to measure the antineutrino flux and search for the possible existence of one or more additional neutrino types. SoLid is searching for an oscillation pattern in the energy spectrum of the $\bar{\nu_{e}}$'s emitted by the SCK.CEN BR2 reactor at Mol in Belgium. This measurement will provide confirmation or...
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  96. 46. Status and physics prospects of Jinping Neutrino Experiment
    Prof. Jian Tang (Sun Yat-Sen University)
    The China Jinping Underground Laboratory (CJPL), which has the lowest cosmic-ray muon flux and the lowest reactor neutrino flux of any laboratory, is ideal to carry out low-energy neutrino experiments. With two detectors and a total fiducial mass of 2000 tons for solar neutrino physics, the Jinping neutrino experiment will have the potential to identify the neutrinos from the CNO fusion cycles...
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  97. 104. T2HKK - Korean detector for HyperK
  98. 98. T2K neutrino and anti-neutrino oscillation results
    Dr Laura Kormos (Lancaster University)
    T2K is a long-baseline neutrino oscillation experiment sited in Japan, consisting of three main components: the JPARC proton accelerator facility that provides a beam of mainly muon neutrinos; a suite of near detectors, INGRID and ND280, that characterize the neutrino beam prior to oscillations; and Super-Kamiokande that acts as the T2K far detector. The far detector beam information is...
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  99. 51. The T2K ND280 upgrade project
    Masashi Yokoyama (University of Tokyo)
    parallel talk
    The T2K neutrino oscillation experiment established the $\nu_\mu \rightarrow \nu_e$ appearance with only 10\% of the original beam request of $7.8\times10^{21}$ 30 GeV protons on target (p.o.t.). In view of the J-PARC program of upgrades of the beam intensity, the T2K-II proposal requires to run up to $20\times10^{21}$ p.o.t., i.e. an increase in the exposure by more than a factor 10 aimed at...
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  100. 45. WATCHMAN: Neutrino Physics and Non-Proliferation
    Prof. Christopher Mauger (University of Pennsylvania)
    WATCHMAN (Water Cherenkov Monitor of AntiNeutrinos) is an international collaboration whose purpose is to demonstrate the feasibility of using a gadolinium-doped water Cherenkov detector to detect electron anti-neutrinos emitted by distant nuclear reactors. Nuclear reactors produce high fluxes of anti-neutrinos during operation and have been exploited by many experiments during the entire...
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  101. 0. Welcome