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The CONNIE experiment Alexis A. Aguilar-Arevalo ICN-UNAM for the - PowerPoint PPT Presentation

The CONNIE experiment Alexis A. Aguilar-Arevalo ICN-UNAM for the CONNIE collaboration VX Mexican Workshop on Particles and Fields Mazatln, Sinaloa, Mxico, 2 6 November, 2015 Motivation Coherent NeutrinoNucleus Elastic


  1. The CONNIE experiment Alexis A. Aguilar-Arevalo ICN-UNAM for the CONNIE collaboration VX Mexican Workshop on Particles and Fields Mazatlán, Sinaloa, México, 2 – 6 November, 2015

  2. Motivation • Coherent Neutrino–Nucleus Elastic Scattering (CNNES): ➔ for neutrino energies below 50 MeV ➔ SM prediction but never measured! ➔ new tool for neutrino experiments (very short baseline oscillation experiments – low energy) ➔ MeV-neutrino physics has great relevance for energy transport in supernovae ➔ monitor nuclear reactors through their emitted neutrinos ➔ CNNES of solar+atm neutrinos forms an irreducible background to future direct dark matter searches → “neutrino fmoor” . • Unique features of high resistivity CCDs designed by Berkeley Laboratories: • very low energy threshold detectors: 5.5 eV ( σ RMS ~ 1.5 e - ) • large mass compared to regular CCDs • “3D” information: event reconstruction • used in the Dark Energy Survey (DES) experiment and Dark Matter in CCDs (DAMIC) experiment Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 2

  3. Coherent ν -N Elastic Scattering CNNES is a neutral-current interaction. A neutrino of any fmavor scatters ofg a nucleus (eg. Si) transferring some energy in the form of a nuclear recoil. atomic number of mass of the neutron number of the nucleus nucleus the nucleus f ( q ) is the nuclear form factor at momentum transfer q For < 50 MeV the momentum transfer ( q 2 ) is small q 2 R 2 < 1 (R = the radius of the nucleus) within an uncertainty of a few percent. Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 3

  4. Coherent ν -N Elastic Scattering CNNES is a neutral-current interaction. A neutrino of any fmavor scatters ofg a nucleus (eg. Si) transferring some energy in the form of a nuclear recoil. σ T σ T weighted by the reactor antineutrino spectrum Reactor antineutrino fmux. PRD91 (2015) 7, 072001 Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 4

  5. Charge Coupled Device 8 Mpix CCD 2k 4 k Scientifjc CCDs developed by LBNL microsystems LAB ● pixel size of 15 µ m X 15 µ m ● thicker than most CCDs (250 - 675 µ m) ● up to 5.2 gr/CCD ● difgusion → 3D reconstruction → rejection of surface events • CCDs cooled to 140 K to achieve readout noise RMS < 2 e − • Energy threshold of ∼0.05 keVee Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 5

  6. Charge Coupled Device The scattering of the ν with a Si nucleus leads to ionization  ν e Charge carriers are drifted along z direction and collected at CCD gates Charge difguses in x - y plane as it drifts towards the gates We fjt the radial spread of the cluster to estimate its position in z within the CCD bulk Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 6

  7. CCD readout - Noise • Added to each pixel by the output amplifjer during the charge readout. • Gaussian distribution with σ RMS that depends on the Janesick pixel readout time. • Pixel time = 30 µ s ⇒ σ RMS = 1.5e- ≡ 5.5 eV of ionization energy PRD91 (2015) 7, 072001 with 60 Co source without 60 Co source Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 7

  8. Particle identifjcation CCD difgusion alpha particle electron limited muon hit Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 8

  9. CCDs calibration with X-rays Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 9

  10. Difgusion from data X-rays, 250 µ m CCD PRD91 (2015) 7, 072001 Difgusion can be modeled with a symmetric Gaussian distribution with lateral spread from 0 to 0.55 pixels. Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 10

  11. Angra Nuclear Power Plant ~ 160 km Angra II 30 m 200 m Angra I ~ 8% more neutrinos ν lab already installed by Neutrinos Angra Project Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 11

  12. Angra Nuclear Power Plant, Flux Angra-2 is a 3.95 GW th Pressurized Water Reactor (PWR) Emits ~8.7 × 10 20 ν e s -1 ( 2.23 × 10 20 ν e s -1 GW th -1) At 30 m the fmux is ~7.8 × 10 20 ν e cm -2 s -1 .  ν e  ν e  ν e Detector  ν e  ν e  ν e Dominant processes (E release) fjs.frac. ν e /proc ν e /fjs 235 U fjssion 202 MeV 0.56 6.14 3.43 238 U fjssion 205 MeV 0.08 7.08 0.56 239 Pu fjssion 210 MeV 0.30 5.58 1.67 241 Pu fjssion 212 MeV 0.06 6.42 0.38 n-capture on 238 U 202 MeV 0.60 2.00 1.20 T ot: 7.24 <E rel> = 205.24 MeV/fjs Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 12

  13. Expected event rate for the Angra reactor T otal number of events as a function of Energy spectra for expected events in silicon detectors the threshold energy for difgerent quenching factors ~ 28 - 300 eV PRD91 (2015) 7, 072001 1 σ 5 σ nuclear-recoil energy spectrum …... The total number of events as spectrum for detectable events a function of the maximum Expected rate detectable recoil (Q = 1) using quenching factor (event/kg/day) E th = 5.5 eV (1 σ RMS ) ~ 28.3 Q = 0.20 E th = 28 eV (5 σ RMS ) ~ 18.1 Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 13

  14. Forecast • Assuming: • a 52 g detector array (10 CCDs with 650 µ m) • Energy threshold of ~28 eV, signal in 28 – 300 eV window. • the background at sea level using passive shield can be reduced to ~600 events/keV/day/kg, i.e. 8.5 events/day • the rate of expected false positive is 3.18 events/day • Expected running time for difgerent CL for a detector’s mass of 52 g CL [%] T (days) 80 12 90 28 95 45 98 70 99 150 PRD91 (2015) 7, 072001 • We need 150 days of running for a 3 σ detection Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 14

  15. CONNIE collaboration Paraguay Argentina Universidad Nacional de Asunción Centro Atómico Bariloche Universidad del Sur / CONICET Brazil Switzerland Centro Brasileiro de Pesquisas Físicas University of Zurich Universidade Federal do Rio de Janeiro USA Mexico Fermilab National Laboratory Universidad Nacional Autónoma de México About 20 people Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 15

  16. Timeline • First visit in 2011 • Seriously making a plan in 2013 • Installed a prototype in 2014 ➔ Detector Shipping August-September 2014 ➔ Detector installation and fjrst data October-November 2014 (10 grams) ➔ Initial operations supported by experts (from USA and Mexico) ➔ Continuous operation now supported by local team (Brazil) ➔ Full shield assembly completed July-August 2015 ➔ August-September 2015 – more than a full month with reactor ON ➔ September-October 2015 – full month of full reactor OFF • Upgrade to 100 g mass detector (CONNIE100) Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 16

  17. The detector During the installation (Oct-Nov/2014) Monsoon readout system VIB board (signal transport) Vacuum pump Cryocooler T emperature Controller Dewar (holds vacuum) Copper Box (holds CCDs) Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 17

  18. The detector CCDs in the During the installation (Oct-Nov/2014) copper box 15 cm lead Inner Dewar polyethylene (holds vacuum) (half moons) Copper Box Polyethylene inside (at the bottom) Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 18

  19. The detector – First light Phase I: Partial shield (30 cm polyethylene and 5 cm lead) 4 CCDs installed and taking data for background studies since Dec/2014 Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 19

  20. The detector – Full shield 1.75 m Dewar with CCDs Phase II: Full shield (installed July-August 2015) 1.75 m 30 cm 30 cm Lead 15 cm Polyethylene Original design 15 cm lead around 30 cm polyethylene Almost fjnished Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 20

  21. The detector – T aking data T esting the system Finishing the shield Alexis A. Aguilar-Arevalo, ICN-UNAM XV Mexican Workshop on Particles and Fields Mazatlán, Sin. México 2-6 Nov 2015 21

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