An Alternative Design based on Inverse Beta Detection Jim Lund Sandia National Laboratories History The immediate future The 2-3 yr. time frame The beehive.

Slides:



Advertisements
Similar presentations
Dante Nakazawa with Prof. Juan Collar
Advertisements

Simulating Radioactive Decays in Next Generation Geoneutrino Detectors Megan Geen Wheaton College Advisor: Nikolai Tolich August 17, 2011.
Double Chooz: Outer Veto
M. Carson, University of Sheffield, UKDMC ILIAS-Valencia-April Gamma backgrounds, shielding and veto performance for dark matter detectors M. Carson,
A Muon Veto for the Ultra-Cold Neutron Asymmetry Experiment Vince Bagnulo LANL Symposium 2006 Outline ● UCNA Experiment ● Muon background ● Proposed Veto.
M. Carson, University of Sheffield IDM 2004, University of Edinburgh Veto performance for a large xenon detector.
A Muon Veto for the Ultra Cold Neutron Asymmetry Experiment Vince Bagnulo with Dr. Jeff Martin Electrons Ultra Cold Neutrons Cosmic Ray Muons Protons Pions.
Past Experience of reactor neutrino experiments Yifang Wang Institute of High Energy Physics, Beijing Nov. 28, 2003.
ANGRA Neutrino Detector: Preliminary Design Main Concepts and Ideas (and some alternatives) Ernesto Kemp State University at Campinas – UNICAMP Gleb Wataghin.
Prospects for 7 Be Solar Neutrino Detection with KamLAND Stanford University Department of Physics Kazumi Ishii.
LLNL A Sandia and Lawrence Livermore National Laboratories Joint Project Nathaniel Bowden Detection Systems and Analysis Sandia National Laboratories,
Discussion of Proposed mini-TimeCube UH Team: Michelle Alderman, Steve Dye, John Learned, Shige Matsuno, Marc Rosen, Michinari Sakai, Stefanie Smith, Gary.
17 September 2010John Learned at ANT2010 Santa Fe1 Univ. of Hawaii: Steve Dye, John Learned, Shigenobu Matsuno, Marc Rosen, Michinari Sakai, Stefanie Smith,
Lepton physics & weak interactions. The neutrino hypothesis Given that you can only measure What physics observations/measurements prompted the addition.
Dec 2005Jean-Sébastien GraulichSlide 1 Improving MuCal Design o Why we need an improved design o Improvement Principle o Quick Simulation, Analysis & Results.
Towards Earth Antineutrino Tomography (EARTH) R.J. de Meijer, F.D. Smit, F.D. Brooks, R.W. Fearick, H.J. Wörtche (EARTH Collaboration) Neutrino Geophysics.
The neutrons detection involves the use of gadolinium which has the largest thermal neutron capture cross section ever observed. The neutron capture on.
Potassium Geo-neutrino Detection Mark Chen Queen’s University Neutrino Geophysics, Honolulu, Hawaii December 15, 2005.
CRS 7/14/2015 # 1 LLNL This work was partially performed under the auspices of the US Department of Energy by the University of California, Lawrence Livermore.
A feasibility study for the detection of SuperNova explosions with an Undersea Neutrino Telescope A. Leisos, A. G. Tsirigotis, S. E. Tzamarias Physics.
1 The Daya Bay Reactor Electron Anti-neutrino Oscillation Experiment Jianglai Liu (for the Daya Bay Collaboration) California Institute of Technology APS.
Status of Recent Detector Deployment(s) at SONGS December 14, 2007
Lecture 15: Beta Decay 23/10/2003 Neutron beta decay: light particles or “leptons”, produced in association. Neutrino presence is crucial to explain.
KamLAND Experiment Kamioka Liquid scintillator Anti-Neutrino Detector - Largest low-energy anti-neutrino detector built so far - Located at the site of.
Geo Neutrino Detection at KamLAND F.Suekane RC S Tohoku University 5th Workshop on Applied Antineutrino Physics (AAP2009) Angra dos Reis, Brazil 20/03/2009.
Interactions of Neutrons
Background from the NIST test The pencil neutron beam (1 mm 2 ) with intensity about 7000 n/sec The beam was completely absorbed in the beam stop with.
R.Svoboda, U.C. Davis /LLNL This work was performed under the auspices of the U.S. Department of Energy by University of California, Lawrence Livermore.
Using Reactor Anti-Neutrinos to Measure sin 2 2θ 13 Jonathan Link Columbia University Fermilab Long Range Planning Committee, Neutrino Session November.
Neutron scattering systems for calibration of dark matter search and low-energy neutrino detectors A.Bondar, A.Buzulutskov, A.Burdakov, E.Grishnjaev, A.Dolgov,
RENO and the Last Result
SNS2 Workshop August 28-29, 2003 Richard Talaga, Argonne1 Calibration of the OMNIS-LPC Supernova Neutrino Detector Outline –OMNIS Experiment and Detectors.
νeνe νeνe νeνe νeνe νeνe νeνe Distance (L/E) Probability ν e 1.0 ~1800 meters 3 MeV) Reactor Oscillation Experiment Basics Unoscillated flux observed.
1 Nuclear Stability The larger the atom, the greater the proportion of the nucleus that must be neutrons. –The A/Z ratio is greater than 2 (or the N to.
2007-DEC-13AAP Prospects for the Use of Large Water- Based Anti-neutrino Detectors for Monitoring Fission Bomb Detonations AAP DEC-13 Eugene.
LSc development for Solar und Supernova Neutrino detection 17 th Lomonosov conference, Moscow, August 2015 L. Oberauer, TUM.
J.T. White Texas A&M University SIGN (Scintillation and Ionization in Gaseous Neon) A High-Pressure, Room- Temperature, Gaseous-Neon-Based Underground.
1 IDM2004 Edinburgh, 9 september 2004 Helenia Menghetti Bologna University and INFN Study of the muon-induced neutron background with the LVD detector.
Neutron detection in LHe ( HMI run 2004) R.Golub, E. Korobkina, J. Zou M. Hayden, G. Archibold J. Boissevain, W.S.Wilburn C. Gould.
1 水质契仑科夫探测器中的中子识别 张海兵 清华大学 , 南京 First Study of Neutron Tagging with a Water Cherenkov Detector.
Experimental Nuclear Physics Some Recent Activities 1.Development of a detector for low-energy neutrons a. Hardware -- A Novel Design Idea b. Measure the.
5 October 2012mTC at AAP20121 John Learned Univ. of Hawaii The mini-Time-Cube A Portable Directional Anti-Neutrino Detector With credits to all the UH.
The Daya Bay Reactor Neutrino Experiment R. D. McKeown Caltech On Behalf of the Daya Bay Collaboration CIPANP 2009.
Performance Comparisons of Safeguard Detector Designs D. Reyna (Argonne National Laboratory) with help from R.W. McKeown (Drexel University)
MaGe framework for Monte Carlo simulations MaGe is a Geant4-based Monte Carlo simulation package dedicated to experiments searching for 0 2  decay of.
Muon and Neutron Backgrounds at Yangyang underground lab Muju Workshop Kwak, Jungwon Seoul National University 1.External Backgrounds 2.Muon.
Karsten Heeger Beijing, January 18, 2003 Design Considerations for a  13 Reactor Neutrino Experiment with Multiple Detectors Karsten M. Heeger Lawrence.
Medical applications of particle physics General characteristics of detectors (5 th Chapter) ASLI YILDIRIM.
Muon flux at Y2L and reconstruction of muon tracks
Daya Bay Reactor Neutrino Experiment On behalf of the DayaBay collaboration Virginia Polytechnic Institute and State University Joseph ykHor YuenKeung,
J-PARC でのハイパー核ガンマ線分光実験用 散乱粒子磁気スペクトロメータ検出器の準備 状況 東北大理, 岐阜大教 A, KEK B 白鳥昂太郎, 田村裕和, 鵜養美冬 A, 石元茂 B, 大谷友和, 小池武志, 佐藤美沙子, 千賀信幸, 細見健二, 馬越, 三輪浩司, 山本剛史, 他 Hyperball-J.
1 Muon Veto System and Expected Backgrounds at Dayabay Hongshan (Kevin) Zhang, BNL DayaBay Collaboration DNP08, Oakland.
1 LTR 2004 Sudbury, December 2004 Helenia Menghetti, Marco Selvi Bologna University and INFN Large Volume Detector The Large Volume Detector (LVD)
Recent Results from RENO NUFACT2014 August. 25 to 30, 2014, Glasgow, Scotland, U.K. Hyunkwan Seo on behalf of the RENO Collaboration Seoul National University.
May 26-27, 2005Tadashi Nomura (Kyoto U), KRare05 at Frascati, Italy1 KOPIO Beam Catcher Tadashi Nomura (Kyoto U.) Contents –What is Beam Catcher? –Concept.
Quesly Daniel, Jr. Florida A&M University Dr. Calvin Howell Duke University, TUNL David Ticehurst UNC-Chapel Hill, TUNL Software for Neutron Detector Capture.
SIMULATION OF BACKGROUND REDUCTION TECHNIQUES FOR Ge DBD DETECTORS Héctor Gómez Maluenda. University of Zaragoza. GERDA/Majorana MC Meeting.
CHANDLER Detector Neutronics Modeling Alireza Haghighat William Walters Nuclear Science and Engineering Lab (NSEL) Nuclear Engineering Program, Mechanical.
Double Chooz Experiment Status Jelena Maricic, Drexel University (for the Double Chooz Collaboration) September, 27 th, SNAC11.
Fast neutron flux measurement in CJPL
SoLid: Recent Results and Future Prospects
The 2nd international conference on particle physics and astrophysics
Calibration, Simulations, and “Remaining” Issues
Neutral Particles.
XAX Can DM and DBD detectors combined?
Tadashi Nomura (Kyoto U), KRare05 at Frascati, Italy
D. Svirida for the DANSS Collaboration (ITEP-JINR)
Signal and Background in LENS
Status of Neutron flux Analysis in KIMS experiment
The Development of a Segmented Detector using ZnS:Ag/6Li
Presentation transcript:

An Alternative Design based on Inverse Beta Detection Jim Lund Sandia National Laboratories History The immediate future The 2-3 yr. time frame The beehive Summary Applied Antineutrino Physics Workshop This work supported by the United States Department of Energy under contract number DE-AC04-94AL Sandia is a multi-program laboratory operated by Sandia Corporation, a Lockheed-Martin Company, for the United States Department of Energy.

History Our first generation detector –Conservative design –It works! –Inefficient –Big

Immediate Future The next generation detector –To be deployed quickly (mid 2007) –More efficient –A straightforward extension of existing work –Much better electronics –Probably a Gd loaded scintillator with better optics and more hermetic muon veto

Intermediate future (2 to 3 yr.) –My pitch! –A relatively advanced inverse beta design –Smaller! –More efficient!

Proposed Design for 2 to 3 yr. Timeframe “The Beehive” Liquid scintillator (~1 m 3 ) Honeycomb partition immersed in liquid scintillator Thin acrylic honeycomb coated with 6 LiF:ZnS(Ag) scintillator Read out with ~100 PMTs

ZnS(Ag) scintillator with 6 Li loading Liquid organic scintillator with pulse shape discrimination ~10 cm ~ 1 m Proposed Design A single voxel

A neutrino hit in the proposed design ZnS(Ag) scintillator with 6 Li loading e+e+ n Neutrino interaction signature –Positron one cell (discounting annihilation photons) Electron-like event in liquid scintillator (fast pulse decay) –Neutron Bright ZnS pulse in two adjacent cells about ~10  s after positron

Background events Fast neutron enters detector Existing Detector Mimics antineutrino capture –Pulse from n-p scatter –Followed by n-capture on Gd Proposed Detector Cut because: –n-p scatter distinguishable from pulse shape

Background events fast neutron into detector Neutrino-like event Background event (fast neutron capture)

Background events slow neutron into detector coincident with gamma ray Existing Detector Mimics antineutrino capture –Pulse from n-p scatter –Followed be n-cature on Gd Proposed Detector Cut because: Gamma event very unlikely to be in same cell as neutron event

Background events two chance gamma-rays within time window Existing Detector Mimics antineutrino capture Proposed Detector Cut because: No signal from ZnS scintillator gammas do not deposit enough energy in ZnS and light from neutron on Li is very large = Q= 4.8 MeV Light pulses from more than one cell

Beehive Detector More efficient than existing detector –Due to ~100% effiency of neutron capture reaction in 6 LiF:ZnS(Ag) scintillator Greater background rejection –Phase space of signal cuts is much richer; easier to classify events Spatial, pulse shape,and two types of scintillator

But Wait, There’s More! Some directionality! ZnS(Ag) scintillator with 6 Li loading e+e+ n e+e+ n

But Wait, There’s More! Some directionality! Although neutron diffusion is a random walk, a slowing neutron preserves a memory (if sloppy) of its original momentum. This property has been observed and exploited in neutrino detection before.

A recent experiment PMT LiF/ZnS(Ag) Scintillator PMT n Trans-Stilbene 2” single crystal

Summary and Acknowledgements A highly segmented detector with 6 LiF:ZnS(Ag) scintillator partitions looks very attractive for monitoring of reactor antineutrinos. We want to do some design experiments! We are very, very grateful to Sandia National Laboratories for giving us funding to study this concept under a Laboratory Directed Research and Development project: –Project Title: Neutrino Detection Technology Development Project Number: