Blacksburg - October 14, 2006 LENS - The Lattice Architecture Jeff Blackmon (ORNL) on behalf of LENS Collaboration 8% Indium-loaded liquid scintillator.

Slides:



Advertisements
Similar presentations
1 Calor02 Pasadena (USA) March 2002Lino Miramonti - University and INFN Milano Borexino: A Real Time Liquid Scintillator Detector for Low Energy.
Advertisements

Status of XMASS experiment Shigetaka Moriyama Institute for Cosmic Ray Research, University of Tokyo For the XMASS collaboration September 10 th, 2013.
Robert Cooper L. Garrison, L. Rebenitsch, R. Tayloe, R. Thornton.
Prototype of the Daya Bay Neutrino Detector Wang Zhimin IHEP, Daya Bay.
Pulse Shape Analysis with Segmented Germanium Detector Xiang Liu, Max-Planck-Institut für Physik 1.Motivation 2.Pulse properties 3.Analysis procedure 4.Some.
Geant4 simulations for the calorimeter prototypes D. Di Julio, J. Cederkäll, P. Golubev, B. Jakobsson Lund University, Lund, Sweden.
Off-axis Simulations Peter Litchfield, Minnesota  What has been simulated?  Will the experiment work?  Can we choose a technology based on simulations?
30 March Global Mice Particle Identification Steve Kahn 30 March 2004 Mice Collaboration Meeting.
Geant4 simulations for the calorimeter prototypes D. Di Julio, J. Cederkäll, P. Golubev, B. Jakobsson Lund University, Lund, Sweden.
Prospects for 7 Be Solar Neutrino Detection with KamLAND Stanford University Department of Physics Kazumi Ishii.
Alternative Prototype Detector Design D. Reyna Argonne National Lab.
M. Kowalski Search for Neutrino-Induced Cascades in AMANDA II Marek Kowalski DESY-Zeuthen Workshop on Ultra High Energy Neutrino Telescopes Chiba,
A Search for Point Sources of High Energy Neutrinos with AMANDA-B10 Scott Young, for the AMANDA collaboration UC-Irvine PhD Thesis:
Discussion of Proposed mini-TimeCube UH Team: Michelle Alderman, Steve Dye, John Learned, Shige Matsuno, Marc Rosen, Michinari Sakai, Stefanie Smith, Gary.
Energy Reconstruction Algorithms for the ANTARES Neutrino Telescope J.D. Zornoza 1, A. Romeyer 2, R. Bruijn 3 on Behalf of the ANTARES Collaboration 1.
Dec 2005Jean-Sébastien GraulichSlide 1 Improving MuCal Design o Why we need an improved design o Improvement Principle o Quick Simulation, Analysis & Results.
Jun 27, 2005S. Kahn -- Ckov1 Simulation 1 Ckov1 Simulation and Performance Steve Kahn June 27, 2005 MICE Collaboration PID Meeting.
MC Study on B°  J/  ° With J/      °     Jianchun Wang Syracuse University BTeV meeting 03/04/01.
1 EMCal design MICE collaboration meeting Fermilab Rikard Sandström.
Lens ALens B Avg. Angular Resolution Best Angular Resolution (deg) Worst Angular Resolution (deg) Image Surface Area (mm 2 )
A feasibility study for the detection of SuperNova explosions with an Undersea Neutrino Telescope A. Leisos, A. G. Tsirigotis, S. E. Tzamarias Physics.
RF background, analysis of MTA data & implications for MICE Rikard Sandström, Geneva University MICE Collaboration Meeting – Analysis session, October.
A crude (lower limit) estimation of resolution and event rate Development and Construction of an Extensive Air Shower Array in HOU Antonis Leisos, Hellenic.
The CMS Level-1 Trigger System Dave Newbold, University of Bristol On behalf of the CMS collaboration.
Progress of HERD Simulation Ming XU ( 徐明 ), IHEP HERD 2 nd Workshop, IHEP, Beijing 1.
Study of response uniformity of LHCb ECAL Mikhail Prokudin, ITEP.
Apostolos Tsirigotis Simulation Studies of km3 Architectures KM3NeT Collaboration Meeting April 2007, Pylos, Greece The project is co-funded by the.
Development of A Scintillation Simulation for Carleton EXO Project Rick Ueno Under supervision of Dr. Kevin Graham.
Simulation study of RENO-50 Jungsic Park Seoul National University RENO-50 International Workshop June 13-14, 2013 Hoam Faculty House, Korea.
A screening facility for next generation low-background experiments Tom Shutt Laura Cadonati Princeton University.
Measuring the Low Energy Solar Neutrino Spectrum LENS-Sol SNOLAB Workshop, Sudbury, Aug 15, 2005 R. S. Raghavan Virginia Tech.
LENS-CAL I. Barabanov, V. Gurentsov, V. Kornoukhov Institute for Nuclear Research, Moscow and R. S. Raghavan, Virginia Tech LONU-LENS Blacksburg, Oct 15,
Feb 10, 2005 S. Kahn -- Pid Detectors in G4MicePage 1 Pid Detector Implementation in G4Mice Steve Kahn Brookhaven National Lab 10 Feb 2005.
Large Magnetic Calorimeters Anselmo Cervera Villanueva University of Geneva (Switzerland) in a Nufact Nufact04 (Osaka, 1/8/2004)
Jan MDI WS SLAC Electron Detection in the Very Forward Region V. Drugakov, W. Lohmann Motivation Talk given by Philip Detection of Electrons and.
EAS Reconstruction with Cerenkov Photons Shower Simulation Reconstruction Algorithm Toy MC Study Two Detector Configuration Summary M.Z. Wang and C.C.
NESTOR SIMULATION TOOLS AND METHODS Antonis Leisos Hellenic Open University Vlvnt Workhop.
Neutron detector developments at LPC Caen  -delayed neutron detectors  current limitations  future issues Search for new solid scintillators (Neutromania)
TUNL R. B. Vogelaar March 1, 2007 Measuring the complete Solar neutrino spectrum E th =114 keV (95% of pp spectrum) Measure pp- 3% Determine CNO-fraction.
Detection of electromagnetic showers along muon tracks Salvatore Mangano (IFIC)
CEA DSM Irfu Reconstruction and analysis of ANTARES 5 line data Niccolò Cottini on behalf of the ANTARES Collaboration XX th Rencontres de Blois 21 / 05.
MINILENS - A Scalable Prototype Detector for LENS LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS Blacksburg, VA, October Mark Pitt.
Nov Beam Catcher in KOPIO (H. Mikata Kaon mini worksyop1 Beam Catcher in the KOPIO experiment Hideki Morii (Kyoto Univ.) for the KOPIO.
LENS:  LENS Simulations, Analysis, and Results B. Charles Rasco Louisiana State University on behalf of the LENS Collaboration.
Towards a high-resolution fluorescence telescope B. Tomé (LIP) IDPASC School on Digital Counting Photosensors for Extreme Low Light Levels, Lisboa,
June 6, 2006 CALOR 2006 E. Hays University of Chicago / Argonne National Lab VERITAS Imaging Calorimetry at Very High Energies.
Magnetized hadronic calorimeter and muon veto for the K +   +  experiment L. DiLella, May 25, 2004 Purpose:  Provide pion – muon separation (muon veto)
Jun Cao Jan. 18, 2004 Daya Bay neutrino experiment workshop (Beijing) Detector Module Simulation and Baseline Optimization ● Determine module geometric.
By Matthew Kauer First Year Report – 15 June 07 Measurement of 2b2ν Half-Life of Zr96 and Lightguide Studies for SuperNEMO Calorimeter Matthew Kauer UCL.
Radia Sia Syracuse Univ. 1 RICH 2004 Outline:  The CLEO-III RICH Detector  Physics Requirements  CLEO-III RICH at work… Performance of the CLEO-III.
The Luminosity Calorimeter Iftach Sadeh Tel Aviv University Desy ( On behalf of the FCAL collaboration ) June 11 th 2008.
Lucia Bortko | Optimisation Studies for the BeamCal Design | | IFJ PAN Krakow | Page 1/16 Optimisation Studies for the BeamCal Design Lucia.
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.
ZEPLIN III Position Sensitivity PSD7, 12 th to 17 th September 2005, Liverpool, UK Alexandre Lindote LIP - Coimbra, Portugal On behalf of the ZEPLIN/UKDM.
PbWO 4 crystals Calorimeter Liping Gan University of North Carolina Wilmington.
Photon Transport Monte Carlo September 27, 2004 Matthew Jones/Riei IshizikiPurdue University Overview Physical processes PMT and electronics response Some.
PAC questions and Simulations Peter Litchfield, August 27 th Extent to which MIPP/MINER A can help estimate far detector backgrounds by extrapolation.
W Prototype Simulations Linear Collider Physics & Detector Meeting December 15, 2009 Christian Grefe CERN, Bonn University.
Upgrade of the MEG liquid xenon calorimeter with VUV-light sensitive large area SiPMs Kei Ieki for the MEG-II collaboration 1 II.
 CC QE results from the NOvA prototype detector Jarek Nowak and Minerba Betancourt.
 13 Readout Electronics A First Look 28-Jan-2004.
SoLid: Recent Results and Future Prospects
Simulation for DayaBay Detectors
Hadronic Shower Structure in WHCAL Prototype
Jin Huang Los Alamos National Lab
A First Look J. Pilcher 12-Mar-2004
Signal and Background in LENS
GEANT Simulations and Track Reconstruction
The Development of a Segmented Detector using ZnS:Ag/6Li
Presentation transcript:

Blacksburg - October 14, 2006 LENS - The Lattice Architecture Jeff Blackmon (ORNL) on behalf of LENS Collaboration 8% Indium-loaded liquid scintillator (pseudocumene) High light output >8000 h /MeV Long attenuation length >8m signal #1 signal #2 #1 prompt electron  e energy (  -like) discrimination Buffer up to 10  s Shower Time/space correlation (~6 m) 3 fiducial volume  ~15 tons Indium ~ 500 pp events/yr (50% eff.)  3% measurement in a few years Critical issues: light collection & resolution (space/time) The Basic LENS Concept Crucial breakthrough See next talks

Blacksburg - October 14, 2006 Longitudinal Design: Classic LENS Typically 3”x3” modules (~5m long) with PMTs on ends End view  t  position Energy must be deposited in 2 of 8 neighbors for good discrimination  30 cm localization along length Extensive simulations: Russia, VaTech, ORNL Efficiency ~35%

Blacksburg - October 14, 2006 Monolith segmented with double-pane nylon & trapped air LENS: The Lattice Architecture Fresnel reflections n=1.5  1.0 Laser demonstration at P~2atm Cartoon representation (2D) Full 3D segmentation for LENS Nearly perfect “digital” event localization Antireflective coatings can reduce losses In-loaded scintillator air

Blacksburg - October 14, 2006 A Tale of Two Sims Two independent modeling efforts with somewhat different approaches Decouple optics from background studies (1) Study pe/MeV yield for each geometry (2) Compare pe/PMT distribution Like “real life” Study optical imperfections Reconstruction & trigger development (2) Background studies: E(x)  Fast (1) Track every optical photon

Blacksburg - October 14, 2006 Cascade vs. 2  background (5”x6m) 3 Light output lower than expected »708 pe/MeV (VaTech = 950 pe/MeV) Cascade  Cascade  Radius 40.4% 0.24% Impose 2 very simple cuts 7.8/ton/yr

Blacksburg - October 14, 2006 LENS Design Figures of Merit Cell Size [mm] Cube size [M] pe/ MeV Det. Eff [%] Nu /t In/y Bgd /t In/y S/NM (In) [tons] M (InLS) tons PMTs (3”) (5”) Signal and Background in LENS Christian Grieb, Virginia Tech, October 2006 Excellent agreement with efficiency & background rate (geometric) Still looking at difference in light: 708 pe/MeV vs. 950 pe/MeV

Blacksburg - October 14, 2006 The “Hard Lattice” No trapped air Easier construction More robust Most photons “channeled”  crit ~60  Good event localization Less trapping Greater light output Solid Teflon Segmentation Challenges: How to deal with “spray”? Background rate Trigger logic

Blacksburg - October 14, 2006 Dark current Each  decay fires ~150 PMT’s (5”) Total decay rate ~4MHz (6m) 3 1% of PMTs fire every ~250 ns ~20 decays between and cascade Number of PMTs firing Events All PMTs PMTs with > 2pe Must reject dark current Simple threshold? More elaborate solution?

Blacksburg - October 14, 2006 Effect of threshold on cascade thresholdpe/MeVrms/mean all pe >1pe/PMT >2pe/PMT >3pe/PMT Air gap Total light output > 2x that w/ air gaps Only 1 pe detected by ~276 PMT’s Introduce threshold at varying levels Cascade   All pe’s >2 pe/PMT Threshold hurts energy resolution Light output still better than air gap

Blacksburg - October 14, 2006 Hard lattice results Impose the same 2 cuts 52% 0.48% 40% & 0.24% Double-foil

Blacksburg - October 14, 2006 Towards a better analysis With the most simple cuts, hard lattice performance is worse … … but the jury is still out More sophisticated approaches: »Maximum likelihood »Neural network algorithm 39% 0.35% pe1/pesum We’re currently investigating a larger parameter space

Blacksburg - October 14, 2006 Optical imperfections Specular spike »About average surface normal Specular lobe »About normal of micofacet Diffuse lobe »Lambertian “diffuse” scattering Backscatter spike »About average surface normal Fine segmentation  treatment of optical properties is very important 4 Types of reflection at boundary Little data on optical properties for detector materials »Measurements needed »Parameterized simulations GEANT4 Optics

Blacksburg - October 14, 2006 Lambertian scattering in “ air gap ” 1% diffuse5% diffuse10% diffusespecular Total pe’s not significantly affected Increasing diffuseness rapidly spreads the pe’s Reconstruction difficult “Dark current” problem similar to the “hard lattice” all pe’s  >2pe/PMT

Blacksburg - October 14, 2006 Cascade  5% Lambertian in “ air gap ” Same results ~40% ~0.3% Same analysis assuming  all pe Cascade  What if we impose >2pe/PMT threshold? Similar results are possible Low light yield is more problematic for single 

Blacksburg - October 14, 2006 Summary The LENS concept is robust Hard Lattice Solid teflon segmentation Scintillation Lattice Double-layer nylon lattice Longitudinal Design 3 viable detector designs Modular approach Best potential performance Most straightforward construction Optical properties important Benchmarking simulations to lab data Prototyping

Blacksburg - October 14, 2006 Bremsstrahlung Beta decay rate = 19 kHz/m 3  (100 keV)  (200 keV)  (300 keV) % % %  (400 keV) 0.71 %  (450 keV) 0.88 %  (500 keV) 1.03 % P(E  >40keV) =   51 Hz/m 3 (BS) Fold with Pfeiffer E  spectrum