Prof.
Masato SHIOZAWA
(Kamioka Observatory, ICRR, The University of Tokyo)
31/10/2018, 14:00
Dr
Akira Konaka
(TRIUMF)
31/10/2018, 14:45
Dr
Michael Smy
(University of California, Irvine)
31/10/2018, 15:30
Shoei Nakayama
(Kamioka Observatory, ICRR, University of Tokyo)
31/10/2018, 16:15
Dr
Mark Hartz
(Kavli IPMU (WPI), University of Tokyo/TRIUMF)
31/10/2018, 17:00
Prof.
Mark Messier
(Indiana)
01/11/2018, 08:10
Prof.
Kei Kotake
(Fukukoka)
01/11/2018, 09:20
Shoei Nakayama
(Kamioka Observatory, ICRR, University of Tokyo)
01/11/2018, 09:40
Dr
Shunichi Mine
(University of California, Irvine)
01/11/2018, 11:45
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)
01/11/2018, 12:10
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
-...
Dr
Terao Kazuhiro
(SLAC National Accelerator Laborator)
01/11/2018, 14:00
John Kelley
(University of Madison–Wisconsin)
01/11/2018, 14:00
parallel talk
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...
Dr
Christian Fruck
(Technical University Munich (TUM))
01/11/2018, 14:20
parallel talk
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...
Dr
Micah Groh
(Indiana University)
01/11/2018, 14:30
parallel talk
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...
Minfang Yeh
(Brookhaven National Lab)
01/11/2018, 14:40
Dr
Anushree Ghosh
(Universidad Técnica Federico Santa María)
01/11/2018, 14:50
Mr
Tanner Kaptanoglu
(University of Pennsylvania)
01/11/2018, 15:00
parallel talk
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...
Prof.
Taritree Wongjirad
(Tufts University)
01/11/2018, 15:10
Dr
Sen QIAN
(IHEP,CAS)
01/11/2018, 15:15
parallel talk
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...
Prof.
Jian Tang
(Sun Yat-Sen University)
01/11/2018, 15:55
parallel talk
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...
Prof.
Liangjian Wen
(Institute of High Energy Physics, Chinese Academy of Sciences)
01/11/2018, 16:00
Alexey Lyashenko
(Incom Inc)
01/11/2018, 16:20
Prof.
Livia Ludhova Ludhova
(Forschungszentrum Juelich)
01/11/2018, 16:20
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 and geoneutrinos. Recently, Borexino has released new results concerning comprehensive spectroscopy of the pp-chain solar neutrinos. The talk will brifely...
Jun Kameda
(University of Tokyo)
01/11/2018, 16:40
Prof.
Juan Pablo Yañez
(University of Alberta)
01/11/2018, 16:45
Dr
Thomas Lindner
(TRIUMF)
01/11/2018, 16:55
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...
Stefania Bordoni
(CERN)
01/11/2018, 17:10
parallel talk
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...
Etam Noah
(University of Geneva)
01/11/2018, 17:10
Dr
Karin Gilje
(University of Alberta)
01/11/2018, 18:00
poster
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...
Dr
Yang Zhang
(University of Alberta)
01/11/2018, 18:03
poster
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...
Micah Buuck
(University of Washington - Seattle)
01/11/2018, 18:06
poster
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...
Prof.
Jianming Bian
(UC Irvine)
01/11/2018, 18:09
poster
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...
Dr
Vincent Fischer Fischer
(University of California at Davis)
01/11/2018, 18:12
poster
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,...
Dr
Matthew Geske
(Gonzaga University)
01/11/2018, 18:18
poster
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...
Dr
Huiling Li
(Institute of High Energy Physics)
01/11/2018, 18:21
poster
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...
Dr
CARLO FRANCESCO VIGORITO
(UNIVERSITY and INFN , Torino, Italia)
01/11/2018, 18:24
poster
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....
Mr
Yatian Pei
(The Institute of High Energy Physics (IHEP))
01/11/2018, 18:27
poster
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...
Mr
Jinjing Li
(Tsinghua University)
01/11/2018, 18:33
poster
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...
Dr
Michael Smy
(University of California, Irvine)
02/11/2018, 09:00
Dr
Azusa Gando
(RCNS, Tohoku University)
02/11/2018, 10:05
Dr
CARLO FRANCESCO VIGORITO
(UNIVERSITY & 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))
02/11/2018, 12:15
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
-...
Dr
Chris Marshall
(Lawrence Berkeley National Laboratory)
02/11/2018, 14:00
parallel talk
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.
Dr
Crespo-Anadón José I.
(Columbia University Nevis Laboratories)
02/11/2018, 14:00
parallel talk
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...
Dr
Hannah Rogers
(Colorado State University)
02/11/2018, 14:20
parallel talk
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...
Dr
Christopher Backhouse
(University College London)
02/11/2018, 14:30
parallel talk
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...
Ms
Francesca Stocker
(CERN)
02/11/2018, 14:40
parallel talk
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...
Tomoyo Yoshida
(Tokyo Institute of Technology)
02/11/2018, 14:55
parallel talk
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...
James Sinclair
(U. Bern)
02/11/2018, 15:00
Dan Dwyer
(LBNL)
02/11/2018, 15:15
Mr
Salvatore Davide Porzio
(The University of Manchester)
02/11/2018, 15:20
parallel talk
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...
Dr
Babak Abi
(University of Oxford)
02/11/2018, 16:00
parallel talk
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...
Kevin McFarland
(University of Rochester)
02/11/2018, 16:10
parallel talk
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.
Dr
Hannah Rogers
(Colorado State University)
02/11/2018, 16:20
Dr
Louise Suter
(Fermi National Accelerator Laboratory)
02/11/2018, 16:35
parallel talk
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...
Mr
Adam Roberts
(University of Liverpool), Dr
Kostas Mavrokoridis
(University of Liverpool)
02/11/2018, 16:40
parallel talk
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...
Kevin McFarland
(University of Rochester)
02/11/2018, 17:00
parallel talk
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.
Zelimir Djurcic
(Argonne National Lab)
02/11/2018, 17:00
Prof.
Michael Wilking
(Stony Brook University)
03/11/2018, 09:00
Erin O'Sullivan
(Stockholm University)
03/11/2018, 14:00
Dr
Mark Hartz
(Kavli IPMU (WPI), University of Tokyo/TRIUMF)
03/11/2018, 16:25
Prof.
David Martinez Caicedo
(South Dakota School of Mines and Technology), Prof.
David Martinez Caicedo
(South Dakota School of Mines and Technology)
03/11/2018, 17:25
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...
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...
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...
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...
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...
