Current status of the Double Chooz experiment
Julia Haser (MPIK Heidelberg)
on behalf of the Double Chooz collaboration
ICHEP Valencia, 2014/07/04
Reactor neutrinos and θ
13Pν¯e→ν¯e ≈1−sin2(2θ13)sin2(1.27∆mE231L)
◾ reactor neutrinos:
▸ pure ¯νe
▸ low energies
▸ short baselines
▸ no matter effects
▸ high flux
◾ 2 detector principle (cancel systematics)
◾ θ13measurement w/o parameter degeneracies
◾ DC far detector only: MC as a substitute for the near detector
Julia Haser (MPIK Heidelberg) DC-III @ ICHEP 2014 2014/07/04 1 / 16
Experimental concept
Double Chooz collaboration
Julia Haser (MPIK Heidelberg) DC-III @ ICHEP 2014 2014/07/04 3 / 16
Neutrino detection
◾ inverse beta decay (IBD) reaction
¯
νe+p→e++n
◾ energy threshold of 1.8 MeV
Evis≈Eν−0.8 MeV
◾ coincidence signal:
▸ prompt: e+annihilation+kinetic energy
▸ delayed: neutron capture
★Gd:E
γ≈8 MeV,τ∼30µs(this talk)
★H:E
γ≈2.2 MeV,τ∼200µs
Double Chooz Detector
µ
VETOES◾ Outer Veto: plastic scintillator strips
◾ Inner Veto: liquid scintillator (LAB) with 78 x 8” PMTs
INNER DETECTOR
◾ ν-Target: liquid scintillator PXE+Gd (1 g/l)
◾ γ-Catcher: liquid scintillator PXE (no Gd)
◾ Buffer: transparent mineral oil with 390 x 10” PMTs
Julia Haser (MPIK Heidelberg) DC-III @ ICHEP 2014 2014/07/04 5 / 16
Energy reconstruction
◾ information from lab measurements and detector calibration
1. uniformity correction with a 2D map 2. time stability (data only)
▸ calibrate variation of mean gain
▸ detector response calibration 3. nonlinearity correction (MC only)
▸ readout related
▸ scintillator model related
⇒data to MC agreement over the full energy range
Backgrounds
Visible Energy (MeV) 2 4 6 8 10 12 14 16 18 20 )/250keV-1Rate (day
10-6 10-5 10-4 10-3 10-2
DC-III (Gd-n) Preliminary
Visible Energy (MeV)
0 5 10 15 20 25 30
Entries / 1.0MeV
1 10 102 103
IBD (standard IBD selection)
IBD above 20 MeV (muon Veto at 30 MeV)
IV Tagged DC-III Gd-n PRELIMINARY
Visible Energy (MeV)
2 4 6 8 10 12
Events/0.50 MeV
0 20 40 60 80 100
120 Double Chooz Preliminary
data MC
natural radioactivity
◾ 0.070±0.003 /day
◾ DC-III/DC-II:0.3 correlation distance cut
DC-II: 2012 DC-III: 2014
fast neutrons, stopping-µ
◾ 0.60±0.05 /day
◾ DC-III/DC-II:0.5 OV and IV veto+
reconstruction likelihood veto
β-n emitter (mainly9Li)
◾ 0.97+0.41−0.16/day
◾ DC-III/DC-II:0.8 Li+He likelihood veto
Julia Haser (MPIK Heidelberg) DC-III @ ICHEP 2014 2014/07/04 7 / 16
Backgrounds
Visible Energy (MeV) 2 4 6 8 10 12 14 16 18 20 )/250keV-1Rate (day
10-6 10-5 10-4 10-3 10-2
DC-III (Gd-n) Preliminary
Visible Energy (MeV)
0 5 10 15 20 25 30
Entries / 1.0MeV
1 10 102 103
IBD (standard IBD selection)
IBD above 20 MeV (muon Veto at 30 MeV)
IV Tagged DC-III Gd-n PRELIMINARY
Visible Energy (MeV)
2 4 6 8 10 12
Events/0.50 MeV
0 20 40 60 80 100
120 Double Chooz Preliminary
data MC
natural radioactivity fast neutrons, stopping-µ β-n emitter (mainly9Li)
◾ reactor OFF-OFF background measurement: 7 events (12.9+3.1−1.4 expected)
▸ NBG(OFF) < ∑NBG(ON)with compatibility of 9 % (1.7σ)
⇒constraint on possible unaccounted background
New neutrino selection
PROMPT ENERGY DELAYED ENERGY CORRELATION TIME
DC-II (2012) DC-III
∆Tµ LE: 1 ms, HE: 0.5 s >1 ms prompt energy 0.7 - 12.2 MeV 0.5 - 20 MeV delayed energy 6 - 12 MeV 4 - 10 MeV
∆T 2 - 100µs 0.5 - 150µs
∆R – <1 m
isolation window [−100,+400]µs [−200,+600]µs +improved Light Noise rejection
+improved BG vetoes
◾ benefits from improved active background rejection
▸ wide selection cuts⇒detection systematics reduction
▸ increased S/B (15.6→22)
Julia Haser (MPIK Heidelberg) DC-III @ ICHEP 2014 2014/07/04 8 / 16
Neutrino Candidates
April 2011 – Jan 2013
◾ live-time: 460.7 days
◾ IBD candidates: 17351 (x2 statistics wrt DC-II)
◾ Reactor-off: 7.24 days, 7 candidates
Normalization uncertainties
source uncertainty (%) improvement wrt DC-II
reactor flux 1.7 –
signal detection
∼0.6 -40 %
statistics 0.8 -30 %
backgrounds 0.8 -50 %
total 2.1 -20 %
uncertainty relative to signal prediction
◾
detection systematics decreased by almost x2
◾
improvement not only in BG reduction, but uncertainty
Julia Haser (MPIK Heidelberg) DC-III @ ICHEP 2014 2014/07/04 10 / 16
Reactor Rate Modulation results
◾ measureθ13(slope) and BG rate (intercept) at the same time
▸ background model independentθ13analysis possible
▸ unique to DC: additional reactor off data point
◾ result:
▸ sin22θ13=0.090+−0.0340.035 (stat+sys)
▸ B=1.56+−0.180.16 day−1
◾ w/o BG rate constraint result:
▸ sin22θ13=0.060±0.039(stat+sys)
▸ B=0.93+−0.430.36 day−1
Rate + Shape results
0.25 MeVEvents
200 400 600 800 1000 1200
DC-III (n-Gd) Preliminary Livetime: 467.90 days
Background-subtracted data No oscillation Systematic uncertainty
= 0.090
¡13 22 Best fit: sin
= 0.00244 eV2 m2 U at
1 2 3 4 5 6 7 8 9 10
0.25 MeVData / Predicted
0.8 0.9 1.0 1.1 1.2
Visible Energy (MeV)
1 2 3 4 5 6 7 8 9 10
0.25 MeVData - Predicted
-100 -50 0 50
◾ other innovations compared to DC-II
▸ range from 0.5-20 MeV (0.25 MeV bins)
▸ measured238U spectrum in prediction
▸ ∆m2from MINOS 2013(T2K confirmed)
▸ extra bin from 2 reactor off measurement
sin22θ13=0.090+−0.0320.029 (stat+sys) χ2min/dof=52.2/40 (p=9.4 %) BG rate after fit: 1.38±0.14 day−1
Julia Haser (MPIK Heidelberg) DC-III @ ICHEP 2014 2014/07/04 12 / 16
Spectrum distortion (1)
◾ spectral distortion above 4 MeV observed
◾ several crosschecks have shown
▸ θ13measurement is not affected
▸ energy scale atE >4 MeV tested (e.g. n-12C) and as cause disfavoured
▸ unknown background disfavoured
Spectrum distortion (2)
◾ RRM fit with free reactor normalization performed for different energy ranges
◾ excess at 4.25−6 MeV consistent with an unaccounted reactor flux
▸ the significance wrt flux prediction is 3σ with BG constraint from our estimation
◾ data-driven study of this energy region:
▸ correlation of excess with reactor power
▸ not only limited to n-Gd sample
Julia Haser (MPIK Heidelberg) DC-III @ ICHEP 2014 2014/07/04 14 / 16
Near detector outlook
◾ detector construction finished
◾ filling this summer
⇒neutrinos in Sept/Oct
◾ 1σwithin [0.015,0.010] after 3 years of ND+FD
▸ BG uncertainty dependent
→statistics dominated!
Summary
◾ DC-III improvements
▸ x2 more statistics
▸ improved energy reconstruction (non-linearities calibrated)
▸ new selection, active BG rejection→increased efficiency, lower systematics
▸ reduced uncertainty on backgrounds, BG estimations fully based on data
▸ 7.24 days of reactor off-off
◾ θ13 results
▸ R+S: sin22θ13=0.090+0.032−0.029, BG rate: 1.38±0.14 day−1
▸ RRM: sin22θ13=0.090+0.034−0.035, BG rate: 1.56±0.17 day−1
▸ RRM (no BG constraint): sin22θ13=0.060±0.039, BG rate: 0.93±0.40 day−1
◾ deviation from reactor flux prediction observed at high energies
◾ ND ready end of summer 2014
▸ targeted 1σ≥0.01 uncertainty on sin22θ13(n-Gd only)
new publication! arxiv: 1406.7763
Julia Haser (MPIK Heidelberg) DC-III @ ICHEP 2014 2014/07/04 16 / 16
Appendix
2014/07/04 18
Energy scale
Visible Energy (MeV) 1 1.2 1.4 1.6 1.8 2 2.2 2.4 2.6 2.8 3
Entries/ 50 keV
0 100 200 300 400 500 600
700 DC-III (Gd-n) Preliminary
data MC
Accidental background
Correlation Distance (m) 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 )/2.5cm-1Rate (day
10-3
10-2
10-1
1
DC-III (Gd-n) Preliminary Data MC Accidentals
2014/07/04 20
Active background reduction
R + S results
2014/07/04 22
Reactor off-off
Visible Energy (MeV)
0 5 10 15 20
)-1MeV-1Background Rate (day
-0.2 -0.1 0 0.1 0.2 0.3 0.4
BG model
2-Off BG
DC-III (n-Gd) Preliminary
◾ 7.24 days of both reactors off→background-only measurement
◾ agreement between reactor off-off and background model
◾ compatibility ofNBG(OFF)and∑NBG(ON)is 9 % (1.7σ)
⇒disfavours unaccounted background
Carbon-12 n-captures
Visible Energy (MeV)
4.0 4.5 5.0 5.5 6.0
Entries/40 keV
200 250 300 350 400 450 500 550 600
DC-III (Gd-n) Preliminary Data
Visible Energy (MeV)
4.0 4.5 5.0 5.5 6.0
Entries/40 keV
500 1000 1500 2000 2500
DC-III (Gd-n) Preliminary MC
◾ n-C peak in Gamma-Catcher with ∆(data,MC) <0.5 %
2014/07/04 24
E/L structure
Visible Energy (MeV)
1 2 3 4 5 6 7 8
0.25 MeVData / Predicted
0.8 0.9 1.0 1.1
1.2 Gd-III data (2014) Gd-II data (2012) H-II data (2012) No oscillation Gd-III best fit
Double Chooz Preliminary Background subtracted
◾ same pattern observed in DC-II results with different detection channels (Gd, H) and detector volumes (Target and Gamma-Catcher)
◾ better resolved with DC-III(more statistics, better energy scale and less background)