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STEREO

D. Lhuillier, CEA - Saclay

D. Lhuillier - AAP 2015 - Arlington VA

1

07/12/2015

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ILL Site

D. Lhuillier - AAP 2015 - Arlington VA

2

07/12/2015

ILL site, Grenoble - France:

  • 57 MW, compact core < 1m
  • [8.9–11.1] m from core, possible extension to 12.3 m.
  • High level of reactor background
  • 15 mwe overburden

No oscillation

First cell

Last cell

Goal: look for relative spectrum distortions in identical cells

6 target cells

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Strategy of the Stereo Measurement

D. Lhuillier - AAP 2015 - Arlington VA

3

07/12/2015

  • Oscillation pattern based on relative shape in identical cells
    • Take advantage of Gd-doped liquid scintillator technology to measure accurate spectra shape.

  • Cosmic rays induced background is the final limitation:
    • Overburden from water channel
    • Online rejection using PSD (stat)
    • Subtraction of residual background using reactor OFF periods (syst)

  • Massive shielding against reactor induce accidentals (stat uncertainty)

  • Sensitive test of the sterile neutrino hypothesis
  • New reference measurement of pure 235U neutrino spectrum.

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Detector Design

D. Lhuillier - AAP 2015 - Arlington VA

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07/12/2015

Reflective plates to suppress dependence on vertex position

Double wall vessel

Central cells in acrylic, filled with Gd-doped LS (90 x 90 x 37.5 cm)

PMTs coupled to LS via a thick acrylic buffer for a better homogeneity

Outer crown (no Gd) to improve energy reconstruction and detection efficiency

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Detector Design

D. Lhuillier - AAP 2015 - Arlington VA

5

07/12/2015

  • Detector vessel is built. Working on top lid machining and inner coating
  • The acrylic buffers will be delivered this week
  • Delivery of all remaining components expected on late February 2016
  • Assembly at CNRS-LPSC in Grenoble before transportation to ILL in April 2016.

Detector vessel

Acrylic buffers

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Liquid Scintillator

D. Lhuillier - AAP 2015 - Arlington VA

6

07/12/2015

  • LAB 75% → protons target
  • PXE 20% + DIN 5% → light yield and PSD
  • Gd-complex 0.2% + 1 %THF → neutron capture
  • PPO + Bis-MSB → wavelength shifters

λ ≳ 5 m

Stable

Transparent

proton recoilsc

electron recoils

PSD

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PMTs

D. Lhuillier - AAP 2015 - Arlington VA

7

07/12/2015

  • 8” PMT: New Hamamatsu R5912-100 with improved Quantum Efficiency, 30% at 420 nm
  • Tests are handled by MPIK Heidelberg in their Faraday lab
  • New PMTs basis with decoupling system delivered by LPSC-Grenoble
  • All components tested and to be delivered this month.

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Detector Response

D. Lhuillier - AAP 2015 - Arlington VA

8

07/12/2015

  • 400 pe/MeV expected
  • Resolution 11.5% (RMS for 2 MeV positrons)
  • Neutron efficiency 60% with a delayed signal above 5 MeV

  • Outer crown:
    • Reduces the difference on neutrons efficiency between center and border cells to 4%
    • Keep the response to prompt signals identical in central and border cells

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Detector Response

D. Lhuillier - AAP 2015 - Arlington VA

9

07/12/2015

  • Linearity of the PMTs and electronics validated in the physics range of interest.

  • The quenching of low energy recoiling electrons introduces a dependence on the way the total energy of an event is deposited.
  • Circulation of radioactive sources inside and around the detector.

  • Monitoring of the detector response by a set a LEDs.

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Calibration

D. Lhuillier - AAP 2015 - Arlington VA

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07/12/2015

3 light injection points per detector cell

+ 12 in the outer crown

Circulation of radioactive sources in calibration tubes

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Calibration

D. Lhuillier - AAP 2015 - Arlington VA

11

07/12/2015

  • Extra information from the deployment of sources underneath and around the detector vessel. Outer crown can be used to veto Compton events
  • Possibility to tag the direction of a 511 keV γ-ray using a 22Na source coupled with a small LYSO crystal
  • Setup under test with a mockup of the detector vessel.

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Prototype Cell

D. Lhuillier - AAP 2015 - Arlington VA

12

07/12/2015

  • The response of a prototype cell has been tested this year.
  • Same height and width than final config, ½ length.
  • Equipped with acrylic buffer and reflective plates
  • Light signals induced in the whole volume by:
    • Source outside the vessel
    • Movable light diffuser
    • Source in central calibration tube

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Prototype Cell

D. Lhuillier - AAP 2015 - Arlington VA

13

07/12/2015

Heigth (cm)

Detected charge (a.u.)

60Co in central tube

Top

Center

  • Small vertex dependence (~5%):
    • Validates the reflective plates
    • Negligible impact on energy resolution
  • Good agreement with the simulation

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Electronics

D. Lhuillier - AAP 2015 - Arlington VA

14

07/12/2015

  • Dedicated electronics hosted in TCA crate
  • Front-end boards are already tested and validated
    • 8-channel FADC 14 bits 250 MHz sampling
    • Qtot, Qtail, tCFD and pulse
    • Gain x1 and x20 for single PE
    • First level programmable trigger (FPGA) validated with muon veto
  • Trigger board: second level programmable trigger (FPGA) taking into account the 3 detectors : Target cells, outer crown, veto
  • LED driver for light calibration
  • All cards already delivered and tested

TCA crate

Trigger board

Front-end

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Data Acquisition

D. Lhuillier - AAP 2015 - Arlington VA

15

07/12/2015

  • Configuration and data collection done using standard ILL software NOMAD
  • Development of low level driver done at LPSC fully operational
  • Slow-control, monitoring, alarm system under development

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Internal Shielding

D. Lhuillier - AAP 2015 - Arlington VA

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07/12/2015

  • 65 T of lead against external γ-rays
  • 6 T Polyethylene against fast neutrons
  • B4C layers against thermal neutrons
  • Soft Iron + μ Metal layers to shield stray B-field

Muon Veto

Internal shieldings

Magnetic shieldings

Overview

  • Seismic study finalized, Fire study still in progress
  • Muon veto umbrella to tag cosmic ray induced background

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Muon Veto

D. Lhuillier - AAP 2015 - Arlington VA

17

07/12/2015

  • Water-Cerenkov detector
    • 4x2.6x0.25 m3 water + wavelength shifter (4MU)
    • 20 PMTs on the top
    • Tyvek diffuser
  • Results from prototype
    • Excellent overall efficiency 98.5% and stable
    • PMTs mapping to reduce sensitivity to γ-rays
  • Final detector fabricated and soon delivered

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Site Characterization

D. Lhuillier - AAP 2015 - Arlington VA

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07/12/2015

Stereo

Extensive γ, μ and n measurements on site performed in 2014-15:

  • Ge, NaI,3He and fast-n detectors inside various shielding
  • Data analysis coupled simulation of the detector setups
  • MCNPX simulations of the reactor and main neutron lines
  • Energy spectrum and location of all sources
  • Design of shielding to meet the specifications of <100 Hz in prompt window and 1 Hz in delayed window.

Modular PE shielding

Directionality studies

Deconvoluted γ-spectrum

Complete reactor simulations

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Shielding Configuration

D. Lhuillier - AAP 2015 - Arlington VA

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07/12/2015

  • Old “H7” line removed

  • Combination of heavy concrete, lead and B4 barriers to block γ and n fluxes.

STEREO

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Shielding Configuration

D. Lhuillier - AAP 2015 - Arlington VA

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07/12/2015

Neutron absorbers added in neighbor primary casemate

STEREO

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Shielding Configuration

D. Lhuillier - AAP 2015 - Arlington VA

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07/12/2015

Last front wall installed in Sept. 2015

10 cm lead + 10 cm PE

STEREO

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Shielding Configuration

D. Lhuillier - AAP 2015 - Arlington VA

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07/12/2015

Final reinforcement of the side wall foreseen this winter.

STEREO

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Sensitivity

D. Lhuillier - AAP 2015 - Arlington VA

23

07/12/2015

  • 400 ν per day during 300 days

  • Signal/Background = 1.5

  • Detection and reconstruction effects from GEANT4 simulation

  • Neutrino flux uncertainties + 4% norm uncertainty

  • Visible Ee+ > 2 MeV

  • En > 5 MeV 🡪 εdet=60%

  • δEscale = 2%

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New Reference 235U Spectrum

D. Lhuillier - AAP 2015 - Arlington VA

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07/12/2015

  • 120 000 ν expected
  • Highly enriched fuel

🡪 pure 235U fission spectrum

Daya Bay Aug. 2015

RENO Nov. 2015

Caution: RENO normalization?

  • Measurement complementary to Double Chooz, Daya Bay and Reno near detectors.

  • Could bring new insight into the deviation at 5 MeV (see Julia’s talk)

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5 MeV Bump

D. Lhuillier - AAP 2015 - Arlington VA

25

07/12/2015

  • Evolution of the sensitivity when introducing the 5 MeV Bump as a new uncertainty in the predicted spectrum (50% of the amplitude).

  • To first order the oscillation phase is not compatible with an isolated deviation around 5 MeV.

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Conclusion

D. Lhuillier - AAP 2015 - Arlington VA

26

07/12/2015

  • Sensitivity contours cover the Reactor Anomaly. Emphasis on control of the detector response to control shape distortions.

  • Final design validated by prototypes and seismic studies

  • Several external shielding walls have already been installed

  • Most parts of detector are under fabrication or already delivered, the schedule is now driven by the delivery of some shielding parts and the final safety agreement.

  • The detector integration will take place at LPSC-Grenoble in Feb-March 2016

  • First data expected in summer 2016