Letter of Interest T2K Experiment
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Book of Abstracts
12th International Neutrino Summer School 2019 Monday 05 August 2019 - Friday 16 August 2019 Fermi National Accelerator Laboratory Book of Abstracts Contents Intro to Group Exercises .................................... 1 Neutrinos and nuclear non-proliferation ........................... 1 INSS2019 welcome and introduction .............................. 1 Solar and Reactor Neutrino Experiments ........................... 1 Precise Measurement of Reactor Antineutrino Oscillation Parameters and Fuel-dependent Variation of Antineutrino Yield and Spectrum at RENO ................. 1 Using Convolutional Neural Networks to Reconstruct Dead Channels in MicroBooNE . 1 Origin and Nature of Neutrino Mass I ............................. 2 Introduction to Leptogenesis .................................. 2 Origin and Nature of Neutrino Mass II ............................ 2 Direct Neutrino Mass Measurements ............................. 2 Neutrinoless Double-beta Decay Experiments ........................ 2 Neutrino Beams and Fluxes .................................. 3 Lepton-Nucleus Cross Section Theory ............................. 3 Neutrino Cross Section Experiments ............................. 3 Origin and Nature of Neutrino Mass III ............................ 3 Particle Astrophysics with High-Energy Neutrinos ..................... 3 Neutrino Detection II ...................................... 3 Phenomenology of Atmospheric and Accelerator Neutrinos ................ 3 Tau neutrinos and upward-going air showers: stochastic versus continuous -
Design and Construction of the Microboone Detector
BNL-113631-2017-JA Design and Construction of the MicroBooBE Detector The MicroBooNE Collaboration Submitted to Journal of Instrumentation January 17, 2017 Physics Department Brookhaven National Laboratory U.S. Department of Energy USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25) Notice: This manuscript has been co-authored by employees of Brookhaven Science Associates, LLC under Contract No. DE-SC0012704 with the U.S. Department of Energy. The publisher by accepting the manuscript for publication acknowledges that the United States Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, nor any of their contractors, subcontractors, or their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or any third party’s use or the results of such use of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof or its contractors or subcontractors. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof. -
The Hunt for Sub-Gev Dark Matter at Neutrino Facilities: a Survey of Past and Present Experiments
Prepared for submission to JHEP The hunt for sub-GeV dark matter at neutrino facilities: a survey of past and present experiments Luca Buonocore,a;b Claudia Frugiuele,c;d Patrick deNivervillee;f aDipartimento di Fisica, Università di Napoli Federico II and INFN, Sezione di Napoli, I-80126 Napoli, Italy bPhysik Institut, Universität Zürich, CH-8057 Zürich, Switzerland cCERN, Theoretical Physics Departments, Geneva, Switzerland dINFN, Sezione di Milano, Via Celoria 16, I-20133 Milano, Italy. eCenter for Theoretical Physics of the Universe, IBS, Daejeon 34126, Korea f T2, Los Alamos National Laboratory (LANL), Los Alamos, NM, USA E-mail: [email protected], [email protected], [email protected] Abstract: We survey the sensitivity of past and present neutrino experiments to MeV-GeV scale vector portal dark matter and find that these experiments possess novel sensitivity that has not yet fully explored. Taking αD = 0:1 and a dark photon to dark matter mass ratio of three, the combined recast of previous analyses of BEBC and a projection of NOνA’s sensitivity are found to rule out the scalar thermal target for dark matter masses between 10 MeV to 100 MeV with existing data, while CHARM-II and MINERνA place somewhat weaker limits. These limits can be dramatically improved by off-axis searches using the NuMI beamline and the MicroBooNE, MiniBooNE or ICARUS detectors, and can even begin to probe the Majorana thermal target. We conclude that past and present neutrino facilities can search for light dark matter concurrently with their neutrino program and reach a competitive sensitivity to proposed future experiments. -
Search for Electron Neutrinos in Multiple Topologies with the Microboone Experiment
Search for Electron Neutrinos in Multiple Topologies with the MicroBooNE Experiment MICROBOONE-NOTE-1085-PUB The MicroBooNE Collaboration June 23, 2020 Abstract This note presents the status of the measurement of electron neutrinos from the Fermilab Booster Neutrino Beamline (BNB) with the MicroBooNE experiment. The analysis is aimed at investigating the nature of the low energy excess of electromagnetic activity observed by the MiniBooNE experiment. The νe event selection relies on topological and calorimetric information to characterise particles produced in these interactions, leveraging the Pandora multi-algorithm reconstruction framework as well as custom particle identification and pattern recognition tools. Results presented in this note use 5:88 × 1020 protons on target of data collected between 2015 and 2018. These include the performance of particle identification tools for µ/p and e/γ separation, along with electromagnetic shower calibration with the largest sample of π0 events measured on argon. Progress towards the completion of this analysis is shown through the measurement of high-energy charged-current νe interactions and their kinematic distributions using both inclusive (1eX) and exclusive (1e0p0π and 1eNp0π) channels. Measurements of charged-current νµ interactions aimed at constraining flux and cross-section systematic uncertainties are also shown. We present the analysis' preliminary sensitivity of an electron-like signal hypothesis to the MiniBooNE excess which includes flux, cross-section, and detector systematic uncertainties. 1 Contents 1 Introduction 3 2 Analysis Approach3 3 Event Reconstruction and Analysis Tools4 4 Electron Neutrino Event Selection7 5 Muon Neutrino Constraint, Systematics, and Analysis Sensitivity 13 6 Selected Electron Neutrinos at High Energy 15 7 Conclusions 16 A Measuring Electron Neutrinos with Particle Identification in the MicroBooNE LArTPC for sensitivity to new Physics 17 B Charged-Current Electron Neutrino Measurement with the MicroBooNE De- tector 20 B.1 Electron identification.................................. -
Arxiv:1804.03238V1 [Hep-Ex] 9 Apr 2018
SNSN-323-63 April 11, 2018 Neutrino Cross Sections: Status and Prospects M. F. Carneiro1 Department of Physics, Oregon State University, Corvallis, Oregon 97331, USA We summarize the current status of accelerator based neutrino cross- section measurements. We focus on the experimental challenges while also presenting the motivation for these measurements. Selected results are highlighted after a quick description of the current major collaborations working on the field. PRESENTED AT arXiv:1804.03238v1 [hep-ex] 9 Apr 2018 NuPhys2017, Prospects in Neutrino Physics Barbican Centre, London, UK, December 20{22, 2017 1This work was supported by NSF Award PHY-1505472. 1 Introduction Neutrino physics is entering a new era of precision measurements and cross section measurements play a vital part. We will not discuss in details the effect of cross section measurements on systematic uncertainties as it has been well described in the literature [1, 2, 3, 4], but rather focus on the experimental difficulties of these measurements as well as show the shortcomings of the current theoretical models de- scribing neutrino-nucleus scattering. We also highlight new results from MINERvA, MicroBooNE, NoVA and T2K which have been released or presented in public con- ferences prior to the time of the NuPhys Workshop (December 2017) as well as given a quick description of each experiment. In Section 1, we discuss the common general goals of the program; in Section 2 we present the experimental difficulties involved in these measurements; Section 3 have a quick description of the effects for oscillation experiments; in Section 4 highlight new results and in Section 5 we summarize and discuss future directions. -
Luke Pickering on Behalf of NUISANCE
nuisance.hepforge.org github.com/NUISANCEMC/nuisance nuisance-xsec.slack.com [email protected] Luke Pickering on behalf of NUISANCE NuSTEC board meeting 2019 ● T2K, MINERvA, DUNE collaborators ● A breadth of experience using GENIE, NuWro, NEUT, GiBUU ● Have worked on neutrino cross-sections measurements, generators dev. and oscillation analyses on T2K and DUNE ● Stared at, thought about, and discussed a lot of neutrino interaction measurements (at NuSTEC and elsewhere) ● Developed interaction systematics for T2K and DUNE analyses ● Started as PhD project, now junior postdocs L. Pickering C. Wret C. Wilkinson ● What is NUISANCE? ● What have we done with NUISANCE? ● What do we plan to do with NUISANCE? ● How can NUISANCE be used in conjunction with NuSTEC? L. Pickering 3 ● Converts generator output from GENIE, NuWro, NEUT, GiBUU and NUANCE ● Uses a common event format with common functions (e.g. GetLepton(), GetQ2(), GetFinalState() ) With all generators in the same format, it’s easy to produce ● Generator-to-generator comparisons ● Model to model comparisons ● Comparison to data ● If event reweighting is available (GENIE, NEUT, NuWro): ○ Fit parameters to data ○ Evaluate uncertainty bands against data ○ Evaluate uncertainties against each other JINST 12 (2017) no. 01, P01016 L. Pickering 4 Compare effect of systematics on distributions from the same generator Effect of MAQE on generated NuWro events versus MiniBooNE CCQE data L. Pickering 5 Compare different generators and their models in a “flat-tree” format CC0π final state from NuWro with Nieves 2p2h CC0π final state from GENIE with Empirical 2p2h L. Pickering 6 Compare your favourite generators and models, which does best/worst? L. -
Session: Neutrino Astronomy
Session: Neutrino Astronomy Chair: Takaaki Kajita, Institute for Cosmic Ray Research, Univ. of Tokyo Basic natures of neutrinos Neutrino was introduced in 1930 by W. Pauli in order to save the energy conservation law in nuclear beta decay processes, in which the emitted electron exhibits a continuous energy spectrum. It was assumed that the penetration power of neutrinos is much higher than that of the gamma rays. More than 20 years later, the existence of neutrinos was experimentally confirmed by an experiment that measured neutrinos produced by a nuclear power reactor. Since then, the basic nature of neutrinos has been understood through various theoretical and experimental studies: Neutrinos interact with matter extremely weakly. The number of neutrino species is three. They are called electron-neutrino, muon-neutrino and tau-neutrino. In addition, recent neutrino experiments discovered that neutrinos have very small masses. Observing the Universe by neutrinos (1) Because of the extremely high penetration power of neutrinos, neutrinos produced at the center of a star easily penetrate to the outer space. Theories of astrophysics predict that there are various processes that neutrinos play an essential role at the center of stars. For example, the Sun is generating its energy by nuclear fusion processes in the central region. In these processes, low energy electron neutrinos with various energy spectra are generated. Thus the observation of solar neutrinos directly probes the nuclear fusion reactions in the Sun. Another example is the supernova explosion. While the optical measurements observe an exploding star, what is happening in the central region of the star is the collapse of the core of a massive star. -
Carsten Rott Curriculum Vitae Feb 2018
Carsten Rott Curriculum Vitae Feb 2018 Department of Physics, Sungkyunkwan University, Suwon 16419, Korea Tel: +82-31-290-5902 E-mail:[email protected] Experimental astro-particle physics, particle physics, geophysics, neutri- Research nos physics Focus Languages German, English; Elementary: French, Japanese, and Korean Employment 2017 { 2018 Honorary Fellow at Wisconsin IceCube Particle Astrophysics Center (WIPAC) (Sabbatical), University of Wisconsin Madison, USA 2017 { now Associate Professor, Sungkyunkwan University, Korea 2013 { 2017 Assistant Professor, Sungkyunkwan University, Korea 2016 Visiting Researcher (3-month), University of Tokyo, Japan 2009 { 2013 Senior Fellow of the Center for Cosmology and AstroParticle Physics (CCAPP) (5-year term), The Ohio State University, USA 2008 { 2009 CCAPP Fellow (3-year term), The Ohio State University, USA 2005 { 2008 Postdoctoral Fellow, Pennsylvania State University, USA Education 1998 { 2004 Purdue University, Indiana, USA Ph.D in Experimental Particle Physics (December 2004) Title : \Search for Scalar Bottom Quarks from Gluino Decays" at CDF Thesis Adviser : Prof. Daniela Bortoletto 1995 { 1998 Universit¨atHannover, Hannover, Germany Honors and Awards 2011 Recipient of NSF Antarctica Service Medal 2005 \Fermilab's Result of the Week" (FermiNews, August 11, 2005) 2004 George W. Tautfest Award, Purdue University 1998 { 1999 University of Hannover { Purdue University direct exchange fellowship Funds and Grants 2017 { present NRF Midscale Research Fund (PI), Korea { NRF-2017R1A2B2003666 2017 { present Foreign Facility Fund (PI of 7 sub-PIs) { NRF-2017K1A3A7A09015973 2016 { present NRF SRC Korea Neutrino Research Center (KNRC) (Co-I), Korea 2016 { 2017 NRF Individual Researcher (PI), Korea { NRF-2016R1D1A1B03931688 2013 { present BrainKorea (BK21plus) participant, Korea 2013 { 2016 NRF Individual Researcher (PI), Korea { NRF-2013R1A1A1007068 2013 { 2014 SKKU Intramural Faculty Fund Award, Korea 2013 { 2014 Fermi GI Cycle 6 (Co-I with Prof. -
Strengthening Global Coordination on Large Neutrino Infrastructures”
July 8, 2016 Press Release concerning the 3rd International Neutrino Meeting on Large Neutrino Infrastructures hosted by KEK on the 30-31st of May 2016 “Strengthening global coordination on large neutrino infrastructures” Funding-agency1 and laboratory representatives2 gathered at the 3rd International Meeting on Large Neutrino Infrastructures3 on May 30-31, 2016 at KEK in Tsukuba, Japan to gauge the progress in the global coordination of projects that had been launched during the first and second international meetings4 and to discuss the next steps in the global coordination. The meeting was opened by the 2015 Nobel Prize winner Takaaki Kajita who commented that “Very large-scale experiments will be needed to fully explore neutrino properties. These large-scale experiments will also naturally have astrophysics potential and increase the sensitivity of searches for proton disintegration.” He went on to note that to realise the necessary very large-scale facilities would require “… international coordination and collaboration” and defined the goals of the meeting to be to “… discuss the physics cases and global strategy, including astrophysics and proton decays, which are the part of the aim of this series of meetings; have follow-up discussions of the ICFA Neutrino Panel’s5 roadmap discussion document”6 and to discuss “… the various neutrino experiments, including Hyper- Kamiokande7, toward the realization of an efficient and productive global neutrino program.” In this meeting, the funding-agency and laboratory representatives welcomed the important steps that had been made towards the realisation of the Hyper-Kamiokande (Hyper-K) experiment7. The international proto-collaboration has developed new, high- sensitivity, large-aperture photomultiplier tubes that substantially reduce the total project cost without unduly compromising its potential to address important questions in particle and astroparticle physics and in nucleon decay. -
Arxiv:1109.3262V1 [Hep-Ex] 15 Sep 2011 University of Tokyo, Department of Physics, Bunkyo, Tokyo 113-0033, Japan
Letter of Intent: The Hyper-Kamiokande Experiment | Detector Design and Physics Potential | K. Abe,12, 14 T. Abe,10 H. Aihara,10, 14 Y. Fukuda,5 Y. Hayato,12, 14 K. Huang,4 A. K. Ichikawa,4 M. Ikeda,4 K. Inoue,8, 14 H. Ishino,7 Y. Itow,6 T. Kajita,13, 14 J. Kameda,12, 14 Y. Kishimoto,12, 14 M. Koga,8, 14 Y. Koshio,12, 14 K. P. Lee,13 A. Minamino,4 M. Miura,12, 14 S. Moriyama,12, 14 M. Nakahata,12, 14 K. Nakamura,2, 14 T. Nakaya,4, 14 S. Nakayama,12, 14 K. Nishijima,9 Y. Nishimura,12 Y. Obayashi,12, 14 K. Okumura,13 M. Sakuda,7 H. Sekiya,12, 14 M. Shiozawa,12, 14, ∗ A. T. Suzuki,3 Y. Suzuki,12, 14 A. Takeda,12, 14 Y. Takeuchi,3, 14 H. K. M. Tanaka,11 S. Tasaka,1 T. Tomura,12 M. R. Vagins,14 J. Wang,10 and M. Yokoyama10, 14 (Hyper-Kamiokande working group) 1Gifu University, Department of Physics, Gifu, Gifu 501-1193, Japan 2High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan 3Kobe University, Department of Physics, Kobe, Hyogo 657-8501, Japan 4Kyoto University, Department of Physics, Kyoto, Kyoto 606-8502, Japan 5Miyagi University of Education, Department of Physics, Sendai, Miyagi 980-0845, Japan 6Nagoya University, Solar Terrestrial Environment Laboratory, Nagoya, Aichi 464-8602, Japan 7Okayama University, Department of Physics, Okayama, Okayama 700-8530, Japan 8Tohoku University, Research Center for Neutrino Science, Sendai 980-8578, Japan 9Tokai University, Department of Physics, Hiratsuka, Kanagawa 259-1292, Japan 10 arXiv:1109.3262v1 [hep-ex] 15 Sep 2011 University of Tokyo, Department of Physics, Bunkyo, -
The World Underground Scientific Facilities a Compendium
A. Bettini G. Galilei Physics Department. Padua University INFN. Padua Canfranc Underground Laboratory [email protected] THE WORLD UNDERGROUND SCIENTIFIC FACILITIES A COMPENDIUM Abstract. Underground laboratories provide the low radioactive background environment necessary to explore the highest energy scales that cannot be reached with accelerators, by searching for extremely rare phenomena. I have requested to the Directors of the Laboratories a standard set of questions on the principal characteristics of their laboratory and collected them in this compendium. I included the ideas and plans for short-range developments. However, next-generation structures, such as those for megaton-size detectors, are not discussed. A short version of this work will be published in the Proccedings of TAUP 2007. 1 2 PREFACE . 4 EUROPE...................................................................................................................................... 6 BNO. BAKSAN NEUTRINO OBSERVATORY (RUSSIA)............................................................................ 6 BUL. BOULBY PALMER LABORATORY (UK)....................................................................................... 9 CUPP. CENTRE FOR UNDERGROUND PHYSICS AT PYHÄSALMI (FINLAND)............................................ 11 LNGS. LABORATORI NAZIONALI DEL GRAN SASSO. L’AQUILA (ITALY) ............................................... 13 LSC. LABORATORIO SUBTERRÁNEO DE CANFRANC (SPAIN).............................................................. 16 LSM. LABORATOIRE -
IUPAP Report 41A
IUPAP Report 41a A Report on Deep Underground Research Facilities Worldwide (updated version of August 8, 2018) Table of Contents INTRODUCTION 3 SNOLAB 4 SURF: Sanford Underground Research Facility 10 ANDES: AGUA NEGRA DEEP EXPERIMENT SITE 16 BOULBY UNDERGROUND LABORATORY 18 LSM: LABORATOIRE SOUTERRAIN DE MODANE 21 LSC: LABORATORIO SUBTERRANEO DE CANFRANC 23 LNGS: LABORATORI NAZIONALI DEL GRAN SASSO 26 CALLIO LAB 29 BNO: BAKSAN NEUTRINO OBSERVATORY 34 INO: INDIA BASED NEUTRINO OBSERVATORY 41 CJPL: CHINA JINPING UNDERGROUND LABORATORY 43 Y2L: YANGYANG UNDERGROUND LABORATORY 45 IBS ASTROPHYSICS RESEARCH FACILITY 48 KAMIOKA OBSERVATORY 50 SUPL: STAWELL UNDERGROUND PHYSICS LABORATORY 53 - 2 - __________________________________________________INTRODUCTION LABORATORY ENTRIES BY GEOGRAPHICAL REGION Deep Underground Laboratories and their associated infrastructures are indicated on the following map. These laboratories offer low background radiation for sensitive detection systems with an external users group for research in nuclear physics, astroparticle physics, and dark matter. The individual entries on the Deep Underground Laboratories are primarily the responses obtained through a questionnaire that was circulated. In a few cases, entries were taken from the public information supplied on the lab’s website. The information was provided on a voluntary basis and not all laboratories included in this list have completed construction, as a result, there are some unavoidable gaps. - 3 - ________________________________________________________SNOLAB (CANADA) SNOLAB 1039 Regional Road 24, Creighton Mine #9, Lively ON Canada P3Y 1N2 Telephone: 705-692-7000 Facsimile: 705-692-7001 Email: [email protected] Website: www.snolab.ca Oversight and governance of the SNOLAB facility and the operational management is through the SNOLAB Institute Board of Directors, whose member institutions are Carleton University, Laurentian University, Queen’s University, University of Alberta and the Université de Montréal.