Outline of CALET Presentation at Scineghe Conference

Outline of CALET Presentation at Scineghe Conference

Outline of CALET presentation at SciNeGHE conference Nicola Mori INFN Florence & University of Florence CALET M&S meeting – GSFC – 23 May 2012 The conference ● “Science with the New Generation of High Energy Gamma-ray Experiments” ● 20-22 June 2012, Lecce (Italy) ● From conference website: “The 2012 edition of the SciNeGHE conference will focus on the interplay between studies and measurements concerning high energy gamma ray sources and cosmic rays.” ● http://scineghe2012.le.infn.it/ Plan of the presentation ● Introduction to CALET – The collaboration – The instrument – General performance (energy resolution etc.) ● Expected results – Electrons and positrons – Nuclei – Gamma ● Electron/proton discrimination Italy Participating institutions • University of Siena • University of Florence & IFAC (CNR) • University of Roma Tor Vergata • University of Padova CALET is a CERN Recognized Experiment Japan ● Waseda University ● Yokohama National University ● United States JAXA/Space Environment ● Hirosaki University ● NASA/Goddard Space Flight Center Utilization Center ● Tokyo Technology Inst. ● ● Louisiana State University JAXA/ Institute of Aerospace ● National Inst. of Radiological Sciences ● Washington University in St. Louis and Astronautical Sciences ● High Energy Accelerator Research ● ● University of Denver Kanagawa University, Organization (KEK) ● Aoyama Gakuin University ● Kanagawa University of Human Services ● Shibaura Institute of Technology ● Saitama University ● Institute for Cosmic Ray Research, ● Shinshu University University of Tokyo ● Nihon University ● Ritsumeikan University Payload overview C Instrument overview z y CHD (CHarge Detector) ● 14 pads per view, EJ204 plastic scintillator (polyvyniltoluene, PVT) 2 Bethe-Bloch formula dE/dx ∝ Z (relativistic) Minimum ionizing CHD discriminates particle (MIP) between different |Z| Z=2 ● Electron/proton separation will require a different approach Z=1 W layers IMC (IMaging Calorimeter) PS fiber layers ● 8 layers, 448 polystyrene fibers (1mm section) per view ● W layers above PS fibers (except for 1st layer), variable height ● Total depth ~ 3 X0, ~ 0.1 λ Fiber readout: Hamamatsu H7546B multianode PMT (64 channels) IMC provides particle's track and finely-segmented information about initial development of EM showers TASC (Total AbSorption Calorimeter) ● 12 layers, 16 lead tungstate (PWO) logs (2 cm section) per view ● Homogeneous calorimeter ● Total depth ~ 27 X0, ~ 1.2 λ ● Energy resolution for e± above 100 GeV: ~ 2 % Readout: APD + PD, Hi and Low gain shapers for each → 4 regimes → high dynamic range (0.5 → 107 MIP) TASC provides energy measurement in a wide range and informations about shower development Performances and scientific goals ● Sensitivity: ● Electrons: 1 GeV – 20 TeV ● Hadrons (H → Fe): ~ 10 GeV – 1000 TeV ● Gamma rays: 10 GeV – 10 TeV ● TASC energy resolution: ● Electrons and gamma rays: ~ 2% @ E > 100 GeV ● Protons: ~ 40% @ 1 TeV ● Nuclei: ~ 30% @ 50 GeV/n (12C and 56Fe) ● CHD charge resolution: 15% - 30% (2 ≤ Z ≤ 26) ● e/p rejection power: ~ 105 ● Acceptance: 0.12 m2 sr ● Planned duration: 5 years From test beam @ GSI Electrons from nearby SNR sources (Kobayashi et al. 2004) Dark matter search: electrons+positrons (e++e-) spectrum from Kaluza-Klein Dark Matter annihilation 2yr (BF=40) or 5yr (BF=16) e++e- flux from fermionic DM decay: + - ΨDM →l l ν MDM = 2.5 TeV (solid line) 26 (Ibarra&Tran 2010) ΤDM = 1.5x10 s Dark matter search: gamma rays : EGRET (Sreekumar et al. 1998) ■: EGRET (Strong et al. 2004) DM contribution (Ibarra, Tran & Weniger 2010) Diffuse gamma-ray flux from fermionic DM decay: + - ΨDM →l l ν MDM = 2.5 TeV (solid line) 26 ΤDM = 1.5x10 s Protons and helium Heavier nuclei B/C ratio CALET at work 100 GeV electron 100 GeV proton Geant4 simulations 100 GeV gama ray 50 GeV/n 12C Geant4 simulations -4 2 -1 Φp(1 TeV) ~ 10 (m sr s GeV) -7 2 -1 Φe(1 TeV) ~ 10 (m sr s GeV) If only 1 proton over 1000 is misinterpreted as an electron, we would end up with a 100% contamination in electron flux!! The requirement for CALET is to be able to select electron and proton events such that proton contamination in electron sample is ~ % N sel N ϵ ϵ ϵ 102 = e = e e =10−3 e e =105 Rejection power sel ϵ ϵ p ϵ p N p N p p Selection efficiency.

View Full Text

Details

  • File Type
    pdf
  • Upload Time
    -
  • Content Languages
    English
  • Upload User
    Anonymous/Not logged-in
  • File Pages
    19 Page
  • File Size
    -

Download

Channel Download Status
Express Download Enable

Copyright

We respect the copyrights and intellectual property rights of all users. All uploaded documents are either original works of the uploader or authorized works of the rightful owners.

  • Not to be reproduced or distributed without explicit permission.
  • Not used for commercial purposes outside of approved use cases.
  • Not used to infringe on the rights of the original creators.
  • If you believe any content infringes your copyright, please contact us immediately.

Support

For help with questions, suggestions, or problems, please contact us