Monitoring of stray magnetic fields near the PROSPECT detector
|
|
- Jeremy Robbins
- 5 years ago
- Views:
Transcription
1 Monitoring of stray magnetic fields near the PROSPECT detector Corey Gilbert On behalf of the PROSPECT Collaboration ORNL is managed by UT-Battelle, LLC for the US Department of Energy Next Talk G : Temperature Dependence studies of the 6Li-doped liquid scintillator used in PROSPECT Brennan T Hackett
2 Motivation PROSPECT is a high precision spectrum antineutrino experiment that requires a well characterized background environment because it is operating at surface level Overburden: ~1m.w.e. Challenge: Neutron scattering experiments conducted in high magnetic environments Backgrounds include: Cosmic Gammas Neutrons Magnetic fields Next Talk G : Temperature Dependence studies of the 6Li-doped liquid scintillator used in PROSPECT }Brennan T Hackett!2
3 High Flux Isotope Reactor (HFIR) Polarized Triple Axis Spectrometer Fixed-Incident- Energy Triple-Axis Spectrometer Inner/ Outer Core 85 MW Thermal Power Research Reactor ~93% enriched 235U fuel Very compact core (h=0.6m d=0.4m) ~42% duty cycle allows good background characterization Neutron Powder Diffractomete HB-1 HB-2 PROSPECT HB-3 HB-4 Cold Neutron Experiment Hall WAND Sample Environment Storage Polarized Neutron Development Neutron Residual Stress Mapping Triple axis spectrometer 4-circle Diffractomete!3
4 Magnets at HFIR Superconducting magnets ranging from 5-11 Tesla are used on various beamlines High field magnets (25-30Tesla) are being considered Mag E 8T Vertical Asymmetric Field Cryomagnet Temp Range: 1.7 to 300 K Used on beamlines : CG-2, CG-4C, HB-1, HB-1A, HB-3!4
5 PMT Configuration in PROSPECT Detector Each of the Li-loaded liquid scintillator filled optical segments holds 2 5 PMTs PMTs are known to be sensitive to magnetic fields. Relative magnetic field values over the range of the device need to be assessed Earth s magnetic field is G at ORNL - Declination: -5º 33 30, Inclination: 64º NOAA Magnetic Field Calculator!5
6 Recent Experimental Efforts to Test/Control Magnetic Environments The STEREO Experiment (Neutrino) - arxiv: v1 (2018) Magnetic shield of PMT used in a DAMPE electromagnetic calorimeter (Dark Matter) - arxiv: v4 (2013) Performances investigation and material selection of PMT magnetic shields for the space experiments with GRIS and PING-M instruments (Space) - R M Faradzhaev et al. J. Phys.675 (2016) First Observation of P-odd γ Asymmetry in Polarized Neutron Capture on Hydrogen (Fundamental Symmetries) - arxiv: v1 (2018) Magnetic field effects on the photocathode uniformity of Hamamatsu R7081 photomultiplier tubes (Industry) - NIMA 697(2013) 46!6
7 Helical Orbit Spectrometer (HeliOS) Studies of short lived isotopes Magnetic field needs to be parallel to beam within 1 mrad Monitoring magnetometers are crucial for this type of experiment!7 Wuosmaa, A. NIMA. 2007
8 PMT Sensitivity to Magnetic Field Backgrounds Low-energy electrons travel along a long path in a vacuum to reach the dynodes. Slight magnetic fields distort that trajectory, causing an anode sensitivity variation Hamamatsu PMT 127mm Hamamatsu, PMT Basics and Applications 2007!8 Boyle J., Master s SESAPS Thesis
9 PMT Module Configuration 240 Hamamatsu R6594 (127 mm ø Q.E. 25%) - 10 stage dynode of box & line configuration 68 ET9372B (130 mm ø Q.E. 28%) - 12 stage dynode of linear focused configuration PROSPECT PMTs are fitted with a Hitachi FINEMET magnetic shield - Amorphous metal composed of Nb, B, Fe, Cu!9
10 Magnetic Field Background Characterization Background B-field was measured using a Lakeshore hall probe (HMMT-6J18-VF) before placement of PROSPECT detector Results showed hotspots approaching 2 Gauss PROSPECT Gauss!10 Boyle J., Master s Thesis 2016
11 Current Magnetometer Technology GMN Earth 1fT 1pT 1nT 1µT 1mT Lenz J., Edelstein A., IEEE Sensors Journal 2006!11
12 Adafruit Triple-Axis Magnetometer Model: LSM303DLHC Selectable range: +/- 1.3 G to +/- 8.1 G Magnetic resolution: 2mG Read through Raspberry Pi I2C 20.3 mm 22.9 mm!12
13 Monitoring of Magnetic Field Rx Core triple axis magnetometers Compact LN2 TOP VIEW DAQ Rack Low cost Online monitoring Alert system 3 1 Remote control 2!13
14 Axes Shift Calibration Out of the box, sensors are not calibrated X and Y magnetic fields plotted as magnetometer is rotated about Z axis before and after axis shift is applied. Programmed in python, takes <1 minute Before After!14
15 Axis Magnitude Calibration Metrolab THM1176-LF hall probe used as known value - Range: 8.0 mt - Resolution: 2µT ± - Accuracy: 20µT or 0.2G Sensor s axes are compared to known and shifted to match!15
16 Magnetic Field Magnitude Around PROSPECT Reactor Core 0.6 Scan using Metrolab hall probe DAQ Rack Gauss Varying magnetic field from 0.15 G to 0.6 G Scanned at sensor height (16cm) Hot spot near DAQ 0.1!16
17 Operation of Sensors since Oct 31 Spike correlated to testing ramp up and down of Mag-E (8 T) on HB-2A!17
18 Magnets Used Since Deployment of PROSPECT Detector MAG-B (5T) MAG-A (5T) MAG-H (5T) MAG-E (8T) MAG-G (11T) MAG-D (11T) HB-1A HB-1 HB-2A HB-2C HB-3 CG-2 CG-4C 3/9/18 4/8/18 5/9/18 6/8/18 7/9/18 8/8/18 9/8/18 10/8/18 11/8/18 Reactor ON Reactor OFF!18
19 Conclusions A compact, low cost magnetic monitoring system has been deployed surrounding the PROSPECT detector at HFIR. Sensors show very good stability and sensitivity to background events Me!19
20 Backup Slides!20
21 Effects of various shielding positions!21 Leo, W.R. Techniques for Nuclear and Particle Physics Experiments. 1994
22 Calibration accuracy Metrolab probe average values plotted with sensor data Sensors values are within 0.2 G of Metrolab probe after calibration Solid lines: Adafruit Sensors Dashed lines: Metrolab probe!22
Measuring the neutrino mass hierarchy with atmospheric neutrinos in IceCube(-Gen2)
Measuring the neutrino mass hierarchy with atmospheric neutrinos in IceCube(-Gen2) Beyond the Standard Model with Neutrinos and Nuclear Physics Solvay Workshop November 30, 2017 Darren R Grant The atmospheric
More informationSearch for Sterile Neutrinos with the Borexino Detector
Search for Sterile Neutrinos with the Borexino Detector PANIC 2014 Hamburg on behalf of the BOREXINO Collaboration Institut für Experimentalphysik (Universität Hamburg) Borexino Detector Site 1400 m of
More informationNeutron facilities and generation. Rob McQueeney, Ames Laboratory and Iowa State University
Neutron facilities and generation Rob McQueeney, Ames Laboratory and Iowa State University September 12, 2018 19-Sep-18 Physics 502 2 Neutrons compared to other probes of matter Bulk probe Interacts with
More informationDirect WIMP Detection in Double-Phase Xenon TPCs
Outline PMTs in the XENON dark matter experiment XENON100 and the weekly gain calibration XENON1T and candidates for the light sensors Tests of Hamamatsu R11410 2 Direct WIMP Detection in Double-Phase
More informationPoS(ICHEP2016)474. SoLid: Search for Oscillations with a Lithium-6 Detector at the SCK CEN BR2 reactor
SoLid: Search for Oscillations with a Lithium-6 Detector at the SCK CEN BR2 reactor University of Bristol E-mail: dan.saunders@bristol.ac.uk The disappearance of reactor antineutrinos into a new neutral
More informationStatus of 13 measurement in reactor experiments
Status of 13 measurement in reactor experiments Kwong Lau University of Houston, Houston, TX 7704, USA The status of 13 measurements from Daya Bay, RENO and Double Chooz experiments is reviewed. 1. INTRODUCTION
More informationAn Underground Laboratory for a Multi-Detector Experiment. Karsten Heeger Lawrence Berkeley National Laboratory
Measuring sin 2 2θ 13 with Reactor Antineutrinos at Daya Bay An Underground Laboratory for a Multi-Detector Experiment Karsten Heeger Lawrence Berkeley National Laboratory On behalf of the Daya Bay collaboration
More informationDaya Bay and joint reactor neutrino analysis
Daya Bay and joint reactor neutrino analysis Logan Lebanowski (Tsinghua University) on behalf of the Daya Bay collaboration 2016/11/4 - NNN16, Beijing 1 Contents Daya Bay Reactor Neutrino Experiment Introduction
More informationXMASS: a large single-phase liquid-xenon detector
XMASS: a large single-phase liquid-xenon detector Katsuki Hiraide, the university of Tokyo for the XMASS Collaboration October 3 rd, 2016 IPRD16@Siena, Italy 1 XMASS project XMASS: a multi purpose experiment
More informationThe Nucifer Experiment: Non-Proliferation with Reactor Antineutrinos
The Nucifer Experiment: Non-Proliferation with Reactor Antineutrinos Andi S. Cucoanes1 for the Nucifer Collaboration* * V.M.Bui2, M.Cribier1, A.S.Cucoanes1, M.Fallot2, M.Fechner1, J.Gaffiot1, L.Giot2,
More informationShort baseline neutrino oscillation experiments at nuclear reactors
Short baseline neutrino oscillation experiments at nuclear reactors Christian Buck, MPIK Heidelberg Erice School, Sicily Sept, 17th 2017 Neutrino oscillations = 3 2 1 3 2 1 3 2 1 3 2 1 ν ν ν ν ν ν τ τ
More informationBeam Dump Experiments at JLab and SLAC
Beam Dump Experiments at JLab and SLAC Brief History (E137 at SLAC) BDX at Jefferson Lab Detector and signal Backgrounds Expected Sensitivity Elton S. Smith, Jefferson Lab On behalf of the BDX Collaboration
More informationNeutrino Oscillations
Neutrino Oscillations Supervisor: Kai Schweda 5/18/2009 Johannes Stiller 1 Outline The Standard (Solar) Model Detecting Neutrinos The Solar Neutrino Problem Neutrino Oscillations Neutrino Interactions
More informationLecture 16 Light transmission and optical detectors
Lecture 6 Light transmission and optical detectors Charged particle traversing through a material can generate signal in form of light via electromagnetic interactions with orbital electrons of the atoms
More informationBeam Dump Experiments with Photon and Electron Beams
Beam Dump Experiments with Photon and Electron Beams Electron beams BDX at Jefferson Lab Signal and backgrounds Muon flux measurements Status Elton S. Smith, Jefferson Lab On behalf of the BDX Collaboration
More informationPoS(DIS 2010)058. ATLAS Forward Detectors. Andrew Brandt University of Texas, Arlington
University of Texas, Arlington E-mail: brandta@uta.edu A brief description of the ATLAS forward detectors is given. XVIII International Workshop on Deep-Inelastic Scattering and Related Subjects April
More informationBackground Modeling and Materials Screening for the LUX and LZ Detectors. David Malling Brown University LUX Collaboration AARM Meeting February 2011
Background Modeling and Materials Screening for the LUX and LZ Detectors David Malling Brown University LUX Collaboration AARM Meeting February 2011 1 Summary LUX screening program limits background contributions
More informationOak Ridge National Laboratory, TN. K. Scholberg, Duke University On behalf of the COHERENT collaboration August 2, 2017 DPF 2017, Fermilab
Oak Ridge National Laboratory, TN K. Scholberg, Duke University On behalf of the COHERENT collaboration August 2, 2017 DPF 2017, Fermilab Coherent elastic neutrino-nucleus scattering (CEvNS) n + A n +
More informationReactor On/Off Monitoring with a Prototype of Plastic Anti-neutrino Detector Array (PANDA)
Reactor On/Off Monitoring with a Prototype of Plastic Anti-neutrino Detector Array (PANDA) Yasuhiro Kuroda A, Yo Kato A, Nozomu Tomita A, Ryoko Nakata, Shugo Oguri, Chikara Ito B, Yoshizumi Inoue C, Makoto
More informationAIRFLY: Measurement of the Air Fluorescence induced by electrons
AIRFLY: Measurement of the Air Fluorescence induced by electrons Valerio Verzi INFN Sezione di Roma II For the Airfly collaboration 9 th Topical Seminar on Innovative Particle and Radiation Detectors 23-26
More informationThe COHERENT Experiment: Overview and Update of Results
The COHERENT Experiment: Overview and Update of Results for the COHERENT Collaboration 2016 Fall Meeting of the APS Division of Nuclear Physics, Vancouver, B.C. ORNL is managed by UT-Battelle for the US
More informationNeutron flux measurement using fast-neutron activation of 12 B and 12 N isotopes in hydrocarbonate scintillators
Neutron flux measurement using fast-neutron activation of 12 B and 12 N isotopes in hydrocarbonate scintillators M. M. Boliev E-mail: kchkrv@rambler.ru Yu. F. Novoseltsev R. V. Novoseltseva V. B. Petkov
More informationNeutrino Physics. Neutron Detector in the Aberdeen Tunnel Underground Laboratory. The Daya Bay Experiment. Significance of θ 13
Neutrino Physics Neutron Detector in the Aberdeen Tunnel Underground Laboratory John K.C. Leung Department of Physics, HKU On behalf of CUHK, LBL & IHEP Presented to HKRPS on June 21, 2007 Neutrinos have
More informationWalter C. Pettus University of Wisconsin Madison. Weak Interactions Discussion Group Yale Physics 21 Oct 2013
Walter C. Pettus University of Wisconsin Madison Weak Interactions Discussion Group Yale Physics 21 Oct 2013 Dark Matter and DM- ICE Cosmogenic Activation in DM- ICE O(50 1000 kev ee ) Calibration Pulse
More informationDark Matter Searches with AMS-02. AMS: Alpha Magnetic Spectrometer
Dark Matter Searches with AMS-02 AMS: Alpha Magnetic Spectrometer 2007/2008 Wim de Boer on behalf of the AMS collaboration University of Karlsruhe July, 20. 2004 COSPAR, Paris, W. de Boer, Univ. Karlsruhe
More informationCorrection for PMT temperature dependence of the LHCf calorimeters
Journal of Physics: Conference Series OPEN ACCESS Correction for PMT temperature dependence of the LHCf calorimeters To cite this article: Eri Matsubayashi and the LHCf collaboration 2015 J. Phys.: Conf.
More informationThe Hyper-Kamiodande Project A New Adventure in n Physics
http://hyperk.org The Hyper-Kamiodande Project A New Adventure in n Physics ICNFP2017 Kolymbari, Crete August 26, 17 Alessandro Bravar on behalf of the HK Proto-Collaboration Hyper-K Physics Overview 2
More informationAfter LUX: The LZ Program. David Malling, Simon Fiorucci Brown University APS DPF Conference August 10, 2011
After LUX: The LZ Program David Malling, Simon Fiorucci Brown University APS DPF Conference August 10, 2011 The LZ Program LZ LUX-ZEPLIN LUX (14 U.S. institutions) + new collaborators from ZEPLIN, other
More informationarxiv:hep-ex/ v1 15 Aug 2006
The Double Chooz Experiment 1 Daniel M. Kaplan (for the Double Chooz Collaboration) Illinois Institute of Technology, 3101 South Dearborn Street, Chicago, Illinois, USA arxiv:hep-ex/0608040v1 15 Aug 2006
More informationarxiv: v1 [physics.ins-det] 9 Apr 2018
arxiv:1804.02889v1 [physics.ins-det] 9 Apr 2018 Study of neutron shielding collimators for curved beamlines at the European Spallation Source 1. Introduction V. Santoro 1,2, D. D. DiJulio 1,2, S. Ansell
More informationChemistry Instrumental Analysis Lecture 19 Chapter 12. Chem 4631
Chemistry 4631 Instrumental Analysis Lecture 19 Chapter 12 There are three major techniques used for elemental analysis: Optical spectrometry Mass spectrometry X-ray spectrometry X-ray Techniques include:
More informationNeutron Instruments I & II. Ken Andersen ESS Instruments Division
Neutron Instruments I & II ESS Instruments Division Neutron Instruments I & II Overview of source characteristics Bragg s Law Elastic scattering: diffractometers Continuous sources Pulsed sources Inelastic
More informationMeasurement of nuclear recoil responses of NaI(Tl) crystal for dark matter search
Measurement of nuclear recoil responses of NaI(Tl) crystal for dark matter search Hanwool Joo on behalf of the KIMS-NaI collaboration Department of Physics and Astronomy, 1 Gwanak-ro, Gwanak-gu, Seoul
More information章飞虹 ZHANG FeiHong INTERNATIONAL SCHOOL OF SUBNUCLEAR PHYSICS Ph.D. student from Institute of High Energy Physics, Beijing
章飞虹 ZHANG FeiHong zhangfh@ihep.ac.cn Ph.D. student from Institute of High Energy Physics, Beijing INTERNATIONAL SCHOOL OF SUBNUCLEAR PHYSICS 2012 Erice, 23 June 2 July 2012 1 Before Hunting Introduction
More informationDirectional Measurement of Anti-Neutrinos with KamLAND
Directional Measurement of Anti-Neutrinos with KamLAND Research Center for Neutrino Science, Tohoku University Aoba-ku aramaki aza aoba, Sendai, Miyagi, Japan E-mail: shingo@awa.tohoku.ac.jp I show possibility
More informationMonte Carlo Simulations for Future Geoneutrino Detectors
Monte Carlo Simulations for Future Geoneutrino Detectors Morgan Askins Abstract The main contribution of heat in the earth s mantle is thought to be the radioactive decays of 238 U, 232 T h, and 40 K.
More informationAppendix A2. Particle Accelerators and Detectors The Large Hadron Collider (LHC) in Geneva, Switzerland on the Border of France.
Appendix A. Particle Accelerators and Detectors The Large Hadron Collider (LHC) in Geneva, Switzerland on the Border of France. Prepared by: Arash Akbari-Sharbaf Why Build Accelerators? Probe deeper From
More informationarxiv: v1 [physics.ins-det] 27 Jun 2017
Double Calorimetry System in JUNO Miao He on behalf of the JUNO collaboration arxiv:1706.08761v1 [physics.ins-det] 27 Jun 2017 Institute of High Energy Physics, Beijing hem@ihep.ac.cn Abstract. The Jiangmen
More informationNew Search for Mirror Neutrons at HFIR
New Search for Mirror Neutrons at HFIR Leah Broussard Oak Ridge National Laboratory October 24, 2017 Neutron-Antineutron Oscillations: Appearance, Disappearance, and Baryogenesis (October 23-27, 2017)
More informationCANDLES Experiment Current Status and Future Plan. X. Li for the CANDLES Collaboration
CANDLES Experiment Current Status and Future Plan X. Li for the CANDLES Collaboration 1 Neutrinoless Double Beta Decay (0νββ) 2νββ decay 0νββ decay (A, Z) => (A, Z+2) + 2e - process beyond Standard Model
More informationNeutron Calibration System for the MiniCLEAN Experiment. Lu Feng for the MiniCLEAN collaboration APS April Meeting May 2, 2011
Neutron Calibration System for the MiniCLEAN Experiment Lu Feng for the MiniCLEAN collaboration APS April Meeting May 2, 2011 The MiniCLEAN Experiment Mini Cryogenic Low Energy Astrophysics with Noble
More informationRecent T2K results on CP violation in the lepton sector
Recent T2K results on CP violation in the lepton sector presented by Per Jonsson Imperial College London On Behalf of the T2K Collaboration, December 14-20 2016, Fort Lauderdale, USA. Outline Neutrino
More informationY2 Neutrino Physics (spring term 2017)
Y2 Neutrino Physics (spring term 2017) Lecture 5 Discoveries of the leptons Dr E Goudzovski eg@hep.ph.bham.ac.uk http://epweb2.ph.bham.ac.uk/user/goudzovski/y2neutrino Previous lecture In 1940s, nuclear
More informationBackground Neutron Studies for Coherent Elastic Neutrino-Nucleus Scattering Measurements at the SNS
Background Neutron Studies for Coherent Elastic Neutrino-Nucleus Scattering Measurements at the SNS D. Markoff (NC Central University, Triangle Universities Nuclear Laboratory) For the COHERENT Collaboration
More informationDetectors for astroparticle physics
Detectors for astroparticle physics Teresa Marrodán Undagoitia marrodan@physik.uzh.ch Universität Zürich Kern und Teilchenphysik II, Zürich 07.05.2010 Teresa Marrodán Undagoitia (UZH) Detectors for astroparticle
More informationNew Search for Mirror Neutrons at HFIR
New Search for Mirror Neutrons at HFIR L. J. Broussard Oak Ridge National Laboratory May 17, 2017 2017 International Workshop on Baryon and Lepton Number Violation Search for neutron disappearance Neutron
More informationThe Daya Bay Reactor Neutrino Oscillation Experiment
The Daya Bay Reactor Neutrino Oscillation Experiment Measurement of θ 13 Mixing Parameter Viktor Pěč for the Daya Bay Experiment Collaboration Charles University in Prague EPS HEP09, Neutrino Physics,
More informationNew results from RENO and prospects with RENO-50
New results from RENO and prospects with RENO-50 Soo-Bong Kim KNRC, Department of Physics and Astronomy, Seoul National University, Seoul 151-742, South Korea Abstract RENO (Reactor Experiment for Neutrino
More informationA RICH Photon Detector Module with G-APDs
A RICH Photon Detector Module with G-APDs S. Korpar a,b, H. Chagani b, R. Dolenec b, P. Križan b,c, R. Pestotnik b, A. Stanovnik b,c a University of Maribor, b J. Stefan Institute, c University of Ljubljana
More informationarxiv:physics/ v1 3 Aug 2006
Gamma Ray Spectroscopy with Scintillation Light in Liquid Xenon arxiv:physics/6834 v1 3 Aug 26 K. Ni, E. Aprile, K.L. Giboni, P. Majewski, M. Yamashita Physics Department and Columbia Astrophysics Laboratory
More informationNeutrino oscillation physics potential of Hyper-Kamiokande
Neutrino oscillation physics potential of Hyper-Kamiokande on behalf of the Hyper-Kamiokande Collaboration Queen Mary University of London E-mail: l.cremonesi@qmul.ac.uk Hyper-Kamiokande (Hyper-K) is a
More informationThe XENON1T experiment
The XENON1T experiment Ranny Budnik Weizmann Institute of Science For the XENON collaboration 1 The XENON1T experiment Direct detection with xenon The XENON project XENON1T/nT 2 Quick introduction and
More informationScintillation Detectors
Scintillation Detectors Introduction Components Scintillator Light Guides Photomultiplier Tubes Formalism/Electronics Timing Resolution Elton Smith JLab 2009 Detecto Summer Lecture Series Experiment basics
More informationCurrent status of LUX Dark Matter Experiment
Current status of LUX Dark Matter Experiment by A. Lyashenko Yale University On behalf of LUX collaboration LUX Large Underground Xenon experiment LUX Collaboration: Yale, CWRU, UC Santa Barbara, Brown,
More informationCosmic Ray Physics with the Alpha Magnetic Spectrometer
Cosmic Ray Physics with the Alpha Magnetic Spectrometer Università di Roma La Sapienza, INFN on behalf of AMS Collaboration Outline Introduction AMS02 Spectrometer Cosmic Rays: origin & propagations: Dominant
More informationPoS(TIPP2014)033. Upgrade of MEG Liquid Xenon Calorimeter. Ryu SAWADA. ICEPP, the University of Tokyo
ICEPP, the University of Tokyo E-mail: sawada@icepp.s.u-tokyo.ac.jp The MEG experiment yielded the most stringent upper limit on the branching ratio of the flavorviolating muon decay µ + e + γ. A major
More informationarxiv: v1 [physics.ins-det] 1 Sep 2009
The MEG Spectrometer at PSI Paolo Walter Cattaneo on behalf of the MEG collaboration INFN Pavia, Via Bassi 6, Pavia, I-27100, Italy arxiv:0909.0199v1 [physics.ins-det] 1 Sep 2009 The MEG experiment is
More informationLatest Results from the OPERA Experiment (and new Charge Reconstruction)
Latest Results from the OPERA Experiment (and new Charge Reconstruction) on behalf of the OPERA Collaboration University of Hamburg Institute for Experimental Physics Overview The OPERA Experiment Oscillation
More informationWalter C. Pettus on behalf of the DM- ICE collaboration University of Wisconsin Madison. APS April Meeting Session D11: Dark Matter II 13 April 2013
Walter C. Pettus on behalf of the DM- ICE collaboration University of Wisconsin Madison APS April Meeting Session D11: Dark Matter II 13 April 2013 Before running a dark matter experiment at the South
More informationThe JUNO veto detector system. Haoqi Lu Institute of High Energy physics (On Behalf of the JUNO Collaboration) TIPP2017, May22-26,Beijing
The JUNO veto detector system Haoqi Lu Institute of High Energy physics (On Behalf of the JUNO Collaboration) TIPP2017, May22-26,Beijing 1 The Jiangmen Underground Neutrino Observatory (JUNO) Detector
More informationarxiv: v1 [hep-ex] 14 May 2015
arxiv:1505.03641v1 [hep-ex] 14 May 2015 Recent Results from Daya Bay Reactor Neutrino Experiment B. Z. HU on behalf of the Daya Bay collaboration Department of Physics, National Taiwan University, No.
More informationPHYS 3446 Lecture #12
PHYS 3446 Lecture #12 Wednesday, Oct. 18, 2006 Dr. 1. Particle Detection Ionization Detectors MWPC Scintillation Counters Time of Flight 1 Announcements Next LPCC Workshop Preparation work Each group to
More informationPREX and CREX. R N from Electroweak Asymmetry in Elastic Electron-Nucleus Scattering. Neutron Skin.
http://hallaweb.jlab.org/parity/prex PREX and CREX 08 Pb Horowitz 48 Ca Neutron Skin R N from Electroweak Asymmetry in Elastic Electron-Nucleus Scattering R L 4 6 A ~ 10 PV Q ~ 10 R L PRL 108 (01) 1150
More informationThe next generation dark matter hunter: XENON1T status and perspective
The next generation dark matter hunter: XENON1T status and perspective A. Rizzo a on behalf of the XENON Collaboration Department of Astrophysics, Columbia University in the City of New York, USA Abstract.
More informationarxiv: v1 [physics.ins-det] 23 Oct 2007
1 arxiv:0710.4279v1 [physics.ins-det] 23 Oct 2007 The SuperNEMO double beta decay experiment I. Nasteva on behalf of the SuperNEMO Collaboration School of Physics and Astronomy, University of Manchester,
More informationJohn Ellison University of California, Riverside. Quarknet 2008 at UCR
Cosmic Rays John Ellison University of California, Riverside Quarknet 2008 at UCR 1 What are Cosmic Rays? Particles accelerated in astrophysical sources incident on Earth s atmosphere Possible sources
More informationNATIONAL RESEARCH NUCLEAR UNIVERSITY MEPhI (Moscow Engineering Physics Institute) Laboratory for Experimental Nuclear Physics
NATIONAL RESEARCH NUCLEAR UNIVERSITY MEPhI (Moscow Engineering Physics Institute) Laboratory for Experimental Nuclear Physics http://enpl.mephi.ru/ The RED-100 Search for elastic coherent neutrino scattering
More informationUpdate on Experiments using SoLID Spectrometer
Update on Experiments using SoLID Spectrometer Yi Qiang for SoLID Collaboration Hall A Collaboration Meeting Dec 16, 2011 Overview SoLID: Solenoidal Large Intensity Device High rate capability: allow for
More informationThe Double Chooz Project
The Double Chooz Project Progress and Expected Sensitivity David McKee, KSU 13 17 July 2009 TeVPA @ SLAC Outline I. Neutrino mixing and θ 13 II. Existing θ 13 measurements III. This is hard with a single
More informationOn the possible construction of a Mu2e calibration linac built around a spare Project-X or ILC cryomodule
On the possible construction of a Mu2e calibration linac built around a spare Project-X or ILC cryomodule George Gollin a Department of Physics University of Illinois at Urbana-Champaign 1110 West Green
More informationThe KATRIN experiment
The KATRIN experiment Status and SDS comissioning Philipp Chung-On Ranitzsch for the KATRIN collaboration Insitute for Nuclear Physics, Westfälische Wilhelms-Universität, Münster The KATRIN experiment
More informationThe GERmanium Detector Array
The GERmanium Detector Array n n ν=v p e - e - p Outline: Exp. issues of 0νββ-decay of 76 Ge Concept of GERDA Status of the experiment Summary and conclusions Kevin Kröninger (Max-Planck-Institut für Physik,
More informationNeutron Scattering under Extreme Conditions at the Spallation Neutron Source
Neutron Scattering under Extreme Conditions at the Spallation Neutron Source Jamie Molaison Oak Ridge National Laboratory International Workshop on Synchrotron High Pressure Mineral Physics and Materials
More informationChung-Yao Fellowship 2016 interview
1/12 Chung-Yao Fellowship 2016 interview Hiroki KUSANO Department of Physics and Astronomy, Shanghai Jiao Tong University May 8, 2016 Resume 1 2/12 Personal data Name: Hiroki Kusano Date of birth: Nov
More informationTemperature Dependence Calibration and Correction of the DAMPE BGO Electromagnetic Calorimeter
Temperature Dependence Calibration and Correction of the DAMPE BGO Electromagnetic Calorimeter Yifeng Wei, Zhiyong Zhang, Yunlong Zhang*, Sicheng Wen, Chi Wang, Zhiying Li, Changqing Feng, Xiaolian Wang,
More informationSTUDY ON THE ENERGY RESPONSE OF PLASTIC SCINTILLATION DETECTOR TO MEV NEUTRONS ABSTRACT
STUDY ON THE ENERGY RESPONSE OF PLASTIC SCINTILLATION DETECTOR TO 0.75-14.75 MEV NEUTRONS Jianfu Zhang 1, 2, Xiaoping Ouyang 1, 2, Suizheng Qiu 1, Xichao Ruan 3, Jinlu Ruan 2 1 School of Nuclear Science
More informationThe Compact Muon Solenoid Experiment. Conference Report. Mailing address: CMS CERN, CH-1211 GENEVA 23, Switzerland. First Physics at CMS
Available on CMS information server CMS CR -2009/034 The Compact Muon Solenoid Experiment Conference Report Mailing address: CMS CERN, CH-1211 GENEVA 23, Switzerland 04 February 2009 First Physics at CMS
More informationDark Matter Particle Explorer: The First Chinese Cosmic Ray and Hard γ-ray Detector in Space
SPACE SCIENCE ACTIVITIES IN CHINA Dark Matter Particle Explorer: The First Chinese Cosmic Ray and Hard γ-ray Detector in Space AUTHORS CHANG Jin Key Laboratory of Dark Matter and Space Astronomy, Purple
More informationDUSEL Theory Workshop, OSU April 4, Yuri Kamyshkov/ University of Tennessee
DUSEL Theory Workshop, OSU April 4, 2008 Yuri Kamyshkov/ University of Tennessee email: kamyshkov@utk.edu τ N N 8 10 sec (in vacuum) Sensitivity for free neutron search (observation probability) t obs
More informationThe Daya Bay Reactor Neutrino Experiment
The Daya Bay Reactor Neutrino Experiment Ming-chung Chu The Chinese University of Hong Kong, Hong Kong On behalf of the Daya Bay Collaboration Partial support: CUHK VC Discretionary Fund, RGC CUHK3/CRF/10R
More informationNeutrinos. Why measure them? Why are they difficult to observe?
Outline What is a neutrino? Why do we want to study them? Building a detector to detect the undetectable What does a neutrino detector see? How do you seperate a neutrino signal from the background? Neutrinos
More informationThe relevance of XENON10 constraints in this low-mass region has been questioned [15] C.E. Aalseth et al. arxiv: v1
The relevance of XENON10 constraints in this low-mass region has been questioned [15] C.E. Aalseth et al. arxiv:1001.2834v1 Peter Sorensen LLNL on behalf of the XENON10 Collaboration at UC Davis HEFTI
More informationSolid Xenon Detector R&D
Solid Xenon Detector R&D Jonghee Yoo Fermilab 24 Feb 2012 UCLA Dark Matter Symposium Solid Xenon Scintillation ~100 ev/γ Phonons ~100 mev/ph Ionization ~10 ev/el Why Xenon? No long-lived Xe radio isotope
More informationAMoRE 0 experiment using low temperature 40 Ca 100 MoO 4 calorimeters
AMoRE 0 experiment using low temperature 40 Ca 100 MoO 4 calorimeters Yong-Hamb Kim On behalf of AMoRE collaboration Institute for Basic Science (IBS) Korea Research Institute for Standards and Science
More informationDetectors for the COHERENT neutrino experiment R. Tayloe Indiana U. for the COHERENT collaboration
Detectors for the COHERENT neutrino experiment R. Tayloe Indiana U. for the COHERENT collaboration Outline Physics motivation Experimental overview detectors: CsI NaI LAr Ge LAr CsI Coherent Elastic n-nucleus
More informationPHY326/426 Dark Matter and the Universe. Dr. Vitaly Kudryavtsev F9b, Tel.:
PHY326/426 Dark Matter and the Universe Dr. Vitaly Kudryavtsev F9b, Tel.: 0114 2224531 v.kudryavtsev@sheffield.ac.uk Indirect searches for dark matter WIMPs Dr. Vitaly Kudryavtsev Dark Matter and the Universe
More informationSolar Neutrinos in Large Liquid Scintillator Detectors
Solar Neutrinos in Large Liquid Scintillator Detectors M. Chen Queen s University DOANOW March 24, 2007 Low Energy Solar Neutrinos complete our understanding of neutrinos from the Sun pep, CNO, 7 Be, pp
More informationarxiv: v1 [physics.ins-det] 29 Jun 2011
Investigation of Large LGB Detectors for Antineutrino Detection P. Nelson a,, N. S. Bowden b, a Department of Physics, Naval Postgraduate School, Monterey, CA 99, USA b Lawrence Livermore National Laboratory,
More informationVacuum System of Synchrotron radiation sources
3 rd ILSF Advanced School on Synchrotron Radiation and Its Applications September 14-16, 2013 Vacuum System of Synchrotron radiation sources Prepared by: Omid Seify, Vacuum group, ILSF project Institute
More informationParticle Detectors Tools of High Energy and Nuclear Physics Detection of Individual Elementary Particles
Particle Detectors Tools of High Energy and Nuclear Physics Detection of Individual Elementary Particles Howard Fenker Jefferson Lab May 31, 2006 Outline of Talk Interactions of Particles with Matter Atomic
More informationx Contents Segmented Mirror Telescopes Metal and Lightweight Mirrors Mirror Polishing
Contents 1 Fundamentals of Optical Telescopes... 1 1.1 A Brief History of Optical Telescopes.................... 1 1.2 General Astronomical Requirements..................... 6 1.2.1 Angular Resolution.............................
More informationStudies of the XENON100 Electromagnetic Background
Studies of the XENON100 Electromagnetic Background Daniel Mayani Physik-Institut University of Zurich PhD Seminar PSI, August 26-27, 2015 Searching for elusive particles The main challenge for experiments
More informationDOE SBIR & STTR FY 2019 Phase 1, Release 1 Topics
Source: InternetCoast BUSINESS OPPORTUNITIES web page>>> Letter of Intent Deadline: September 4, 2018 Application Deadline: October 15, 2018 Download Solicitation Topic Details>>> 1. TECHNOLOGIES FOR MANAGING
More informationPublications of Francesco Arneodo: journal articles
Publications of Francesco Arneodo: journal articles Figure 1: Citation report from ISI Web of Science (IF=31.0) [1] E. Aprile et al., First Axion Results from the XENON100 Experiment, arxiv.org (submitted
More informationThe Compact Muon Solenoid Experiment. Conference Report. Mailing address: CMS CERN, CH-1211 GENEVA 23, Switzerland. Commissioning of the CMS Detector
Available on CMS information server CMS CR -2009/113 The Compact Muon Solenoid Experiment Conference Report Mailing address: CMS CERN, CH-1211 GENEVA 23, Switzerland 15 May 2009 Commissioning of the CMS
More information(a) (i) State the proton number and the nucleon number of X.
PhysicsAndMathsTutor.com 1 1. Nuclei of 218 84Po decay by the emission of an particle to form a stable isotope of an element X. You may assume that no emission accompanies the decay. (a) (i) State the
More informationThe Daya Bay Anti-neutrino Experiment
The Daya Bay Anti-neutrino Experiment On behalf on the Daya Bay Collaboration Jianglai Liu Shanghai Jiao Tong University KPS-CPS joint session, KPS annual meeting, Busan, 2011-10-20 1 13 in PMNS Matrix
More informationUCN supersource at PNPI and fundamental physics program А.P. Serebrov
UCN supersource at PNPI and fundamental physics program А.P. Serebrov 8 th UCN Workshop Ultra Cold & Cold Neutrons Physics & Sources 11-21 June 2011 1 Content 1. UCN sources at PNPI 2. Ultracold neutron
More informationP.M. King Ohio University for the MOLLER Collaboration
Parity violating electron scattering at JLab: the MOLLER experiment P.M. King Ohio University for the MOLLER Collaboration SESAPS, 10 November 2016; University of Virginia, Charlottesville, VA The Standard
More informationTHE CRYOGENIC UNDERGROUND OBSERVATORY FOR RARE EVENTS: STATUS AND PROSPECTS
THE CRYOGENIC UNDERGROUND OBSERVATORY FOR RARE EVENTS: STATUS AND PROSPECTS Eric B. Norman Dept. of Nuclear Engineering Univ. of California, Berkeley, CA U. S. A. Recent results in n physics Neutrinos
More information