The ICARUS 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.................................. -
Summary of the Second Workshop on Liquid Argon Time Projection Chamber Research and Development in the United States
FERMILAB-CONF-15-149-ND Preprint typeset in JINST style - HYPER VERSION Summary of the Second Workshop on Liquid Argon Time Projection Chamber Research and Development in the United States R. Acciarria, M. Adamowskia, D. Artripb, B. Ballera, C. Brombergc, F. Cavannaa;d, B. Carlsa, H. Chene, G. Deptucha, L. Epprecht f , R. Dharmapalang W. Foremanh A. Hahna, M. Johnsona, B. J. P. Jones i, T. Junka, K. Lang j, S. Lockwitza, A. Marchionnia, C. Maugerk, C. Montanaril, S. Mufsonm, M. Nessin, H. Olling Backo, G. Petrillop, S. Pordesa, J. Raafa, B. Rebela, G. Sininsk, M. Soderberga;q, N. Spoonerr, M. Stancaria, T. Strausss, K. Teraot , C. Thorne, T. Topea, M. Toupsi, J. Urheimm, R. Van de Waterk, H. Wangu, R. Wassermanv, M. Webers, D. Whittingtonm, T. Yanga aFermi National Accelerator Laboratory, Batavia, IL 60510, USA bResearch Catalytics, USA cMichigan State University, East Lansing, MI 48824, USA dYale University, New Haven, CT 06520, USA eBrookhaven National Laboratory, Upton, NY 11973, USA f ETH Zürich, 8092 Zürich, Switzerland gArgonne National Laboratory, Argonne, IL, 60439, USA hUniversity of Chicago, Chicago, IL 60637, USA iMassachusetts Institute of Technology, Cambridge, MA 02139, USA jUniversity of Texas at Austin, TX 78712, USA kLos Alamos National Laboratory, Los Alamos, NM 87545, USA lIstituto Nazionale di Fisica Nucleare, Pavia 6-27100, Italy mIndiana University, Bloomington, IN 47405, USA nCERN, 1217 Meyrin, Switzerland oPrinceton University, Princeton, NJ 08544, USA pUniversity of Rochester, Rochester, NY 14627, USA qSyracuse University, NY 13210, USA rUniversity of Sheffield, Sheffield, South Yorkshire S10 2TN, UK sUniversity of Bern, 3012 Bern, Switzerland t Columbia University, New York, NY 10027, USA uUniversity of California Los Angeles, Los Angeles, CA 90095, USA vColorado State University, Fort Collins, CO 80523, USA – 1 – Operated by Fermi Research Alliance, LLC under Contract No. -
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. -
An Introduction to Solar Neutrino Research
AN INTRODUCTION TO SOLAR NEUTRINO RESEARCH John Bahcall Institute for Advanced Study, Princeton, NJ 08540 ABSTRACT In the ¯rst lecture, I describe the conflicts between the combined standard model predictions and the results of solar neutrino experi- ments. Here `combined standard model' means the minimal standard electroweak model plus a standard solar model. First, I show how the comparison between standard model predictions and the observed rates in the four pioneering experiments leads to three di®erent solar neutrino problems. Next, I summarize the stunning agreement be- tween the predictions of standard solar models and helioseismological measurements; this precise agreement suggests that future re¯nements of solar model physics are unlikely to a®ect signi¯cantly the three solar neutrino problems. Then, I describe the important recent analyses in which the neutrino fluxes are treated as free parameters, independent of any constraints from solar models. The disagreement that exists even without using any solar model constraints further reinforces the view that new physics may be required. The principal conclusion of the ¯rst lecture is that the minimal standard model is not consistent with the experimental results that have been reported for the pioneering solar neutrino experiments. In the second lecture, I discuss the possibilities for detecting \smok- ing gun" indications of departures from minimal standard electroweak theory. Examples of smoking guns are the distortion of the energy spectrum of recoil electrons produced by neutrino interactions, the de- pendence of the observed counting rate on the zenith angle of the sun (or, equivalently, the path through the earth to the detector), the ratio of the flux of neutrinos of all types to the flux of electron neutrinos 1 (neutral current to charged current ratio), and seasonal variations of the event rates (dependence upon the earth-sun distance). -
ACTA PHYSICA POLONICA B No 6–7
Vol. 35 (2004) ACTA PHYSICA POLONICA B No 6–7 THE ICARUS EXPERIMENT AT THE GRAN SASSO UNDERGROUND LABORATORY∗ ∗∗ A. Zalewska for the ICARUS Collaboration The H. Niewodniczański Institute of Nuclear Physics Polish Academy of Sciences Radzikowskiego 152, 31-342 Kraków, Poland e-mail: [email protected] (Received May 14, 2004) The present ICARUS detector, called T600, is ready for installation in the Gran Sasso underground laboratory. It consists of two large cryostats, each one filled with 300 tons of Liquid Argon and equipped with two Time Projection Chambers (TPCs). An overview of the T600 detector is given. Main results of the analyses of the data collected during the surface tests with cosmic rays in summer 2001 are presented. They illustrate the de- tector’s excellent performance. A vast physics program of the ICARUS experiment, which includes different aspects of the neutrino studies and searches for proton decays, is shortly discussed. Finally, the detector up- grade towards the total mass of 3000 tons of Liquid Argon is mentioned. PACS numbers: 13.20.+g, 14.60.Pq, 29.40.Gx, 29.40.Vj 1. Introduction The ICARUS experiment [1] will be realized at Gran Sasso, in the world’s largest underground laboratory. It is located under 1400 meters of rock and is accessed from the tunnel of the Roma–Teramo highway. There are three big experimental halls and a number of galleries and small chambers. The ICARUS detector will be placed in hall B. The ICARUS detector is based on the concept of large TPC chambers filled with Liquid Argon (LAr), originally proposed by C. -
Pos(Neutel 2013)013
Sterile neutrino search with the ICARUS T600 in the CNGS beam PoS(Neutel 2013)013 PoS(Neutel 2013)013 Robert Sulej 1 National Centre for Nuclear Research A. Soltana 7, 05-400 Otwock, Swierk, Poland E-mail: [email protected] We report an early result from the ICARUS experiment on the search for a νµ→νe signal due to the LSND anomaly. The search was performed with the ICARUS T600 detector located at the Gran Sasso Laboratory, receiving CNGS neutrinos from CERN at an average energy of about 20 GeV, at a distance to source of about 730 km. At the L/E ν = 36.5 m/MeV of the ICARUS experiment the LSND anomaly would manifest as an excess of νe events, characterized by a fast 2 2 energy oscillation averaging approximately to sin (1.27 ∆m new L/E ν) ≈ 1/2 with probability 2 Pνµ →νe = 1/2sin (2θnew ). The present analysis is based on 1091 neutrino events, which are about 50% of the ICARUS data collected in 2010–2011. Two clear νe events have been found, compared with the expectation of 3 .7±0.6 events from conventional sources. Within the range of observations, this result is compatible with the absence of a LSND anomaly. At 90% and 99% confidence levels the limits of 3.4 and 7.3 events, corresponding to oscillation probabilities −3 −2 〈Pνµ →νe〉 ≤ 5.4×10 and 〈Pνµ →νe〉 ≤ 1.1×10 , are respectively set. The result strongly limits the 2 2 2 window of open options for the LSND anomaly to a region around (∆m , sin (2θ)) new = (0.5eV , 0.005), where there is an overall agreement at 90% CL between the present ICARUS limit, the published limits of KARMEN and the published positive signals of LSND and MiniBooNE Collaborations. -
Cosmic Ray Background Rejection with Wire-Cell Lartpc Event Reconstruction in Microboone
Cosmic Ray Background Rejection with Wire-Cell LArTPC Event Reconstruction in MicroBooNE MICROBOONE-NOTE-1084-PUB The MicroBooNE Collaboration∗ (Dated: June 20, 2020) For a large Liquid Argon Time Projection Chamber (LArTPC) operating on or near the surface to detect neutrino interactions, the rejection of cosmic background is a critical and challenging task because of the large cosmic ray flux and the slow timing of the TPC. In this paper, we introduce a superior cosmic background rejection procedure based on the Wire-Cell 3D event reconstruction for LArTPCs. The foundational reconstruction techniques including the 3D imaging and clustering of TPC ionization charge data, processing of PMT light data, and matching of the TPC charge and PMT light information are reviewed. This is followed by a detailed description of track trajectory fitting and dQ=dx determination. These reconstruction tools further enable various methods to tag cosmic-ray muons in time with the neutrino beam spills. From a hardware trigger level 1:20k neutrino to cosmic-ray background ratio, high-performance generic neutrino selection, i.e. cosmic- ray background rejection, is achieved in the MicroBooNE experiment with a cosmic contamination of 14.9% (9.7%) for the visible energy region greater than 0 (200) MeV. High efficiencies of neutrino interactions are also retained, and they are 80.4% and 87.6% for νµ charged-current and νe charged- current interactions, respectively. CONTENTS B. Stopped muon examples 23 I. Introduction 1 References 24 II. MicroBooNE detector and readout 3 I. INTRODUCTION III. Review of foundational reconstruction techniques 4 The liquid argon time projection chamber [1{4] A. -
Long-Baseline Neutrino Oscillation Experiments
Long-Baseline Neutrino Oscillation Experiments The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Feldman, G. J., J. Hartnell, and T. Kobayashi. 2013. “Long-Baseline Neutrino Oscillation Experiments.” Advances in High Energy Physics 2013: 1–30. doi:10.1155/2013/475749. Published Version doi:10.1155/2013/475749 Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:28237456 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Open Access Policy Articles, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#OAP Long-baseline Neutrino Oscillation Experiments G. J. Feldman Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA. E-mail: [email protected] J. Hartnell Department of Physics and Astronomy, University of Sussex, Brighton. BN1 9QH. United Kingdom. E-mail: [email protected] T. Kobayashi Institute for Particle and Nuclear Studies, High Energy Accelerator Research Organization (KEK), 1-1, Oho, Tsukuba, 305-0801, Japan. E-mail: [email protected] Abstract. A review of accelerator long-baseline neutrino oscillation experiments is provided, including all experiments performed to date and the projected sensitivity of those currently in progress. Accelerator experiments have played a crucial role in the confirmation of the neutrino oscillation phenomenon and in precision measurements of the parameters. With a fixed baseline and detectors providing good energy resolution, precise measurements of the ratio of distance/energy (L=E) on the scale of individual events have been made and the expected oscillatory pattern resolved.