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Experiment Neutrino-4 on search for sterile neutrino А. Serebrov
Collaboration Neutrino-4: 1. NRC “KI” Petersburg Nuclear Physics Institute, Gatchinа, NRC 2. “Kurchatov institute”, Moscow, 3. JSC “SSC RIAR”, Dimitrovgrad, Russia 4. DETI MEPhI, Dimitrovgrad, Russia А Serebrov1, V Ivochkin1, R Samoilov1, А Fomin1, A Polyushkin1, V Zinoviev1, P Neustroev1,V Golovtsov1, А Chernyj1, О Zherebtsov1, V Martemyanov2, V Tarasenkov2, V Aleshin2, А Petelin3, А Izhutov3, А Тuzov3, S Sazontov3, D Ryazanov4, М Gromov3, V Afanasiev3, М Zaytsev1, 4, М Chaikovskii1 Международная сессия-конференция Секции ядерной физики ОФН РАН "Физика фундаментальных взаимодействий", посвященная 50-летию Баксанской нейтринной обсерватории 6-8 июня 2017 г.
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The reactor antineutrino anomaly and sterile neutrino
G. Mention et al., Phys. Rev. D83, , 2011 The reactor antineutrino anomaly and sterile neutrino
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Experiment Neutrino-4 at SM-3 reactor
1 Petersburg Nuclear Physics Institute NRC KI, Gatchinа, 2 NRC “Kurchatov institute”, Moscow, 3 JSC “SSC RIAR”, Dimitrovgrad, 4 DETI MEPhI, Dimitrovgrad, SM-3 WWER-1000 100 MW 60 MW 85 MW 20 MW 250 MW Size of active zone of reactor SM-3: 424235 cm 2700 MW 3000 MW Core size and power of different reactors
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Prototype of NEUTRINO-4 detector, 400 l
The model of the neutrino detector installed in passive shielding 1 – detector of reactor antineutrino, 2 – passive shielding, 3 – rail, 4 – the engine for detector movement, 5 – active shielding with PMT, 6 – volume with liquid scintillator liquid with Gd (~ 400 l), 7 – Detector PMT.
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Assembling of electronics for prototype of NEUTRINO-4 detector
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Computer room – data processing
We begin the first measurements on model of the neutrino detector
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Outlay of the neutrino laboratory
(left side - passive shielding of neutrino detector, 60 tons)
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General view of neutrino laboratory
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First version of active shielding
Second version of active shielding External active shielding – "umbrella"
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The problem of fast neutrons
Neutron scattering imitate neutrino reaction
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Multi-section model of detector
liquid scintillator PTM Table 1. The probability of double-start events registration in various sections. central section side section corner section average 0.42 0.29 0.19 0.30 Monte-Carlo calculations
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Multi-section antineutrino detector model
The detector consists of 16 sections 22.5 x 22.5 x 50 cm3 with fixed baffles. The baffles are made of acrylic plastic and have specular surface serve to prevent light from leaving the section. Scintillator material is mineral oil (CH2) with addition of Gadolinium 1g per litter.
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General scheme of installation
. 1 – detector of reactor antineutrino, 2 – internal active shielding, 3 – external active shielding (umbrella), 4 – steel and lead passive shielding, 5 – borated polyethylene passive shielding, 6 – moveable platform, 7 – feed screw, 8 – step motor.
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The full-scale detector with liquid scintillator volume of
3 m3 (5x10 sections) is installed already
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Comparison with calculation
Share of multi starts Comparison with calculation calculation central cell, double coincidence side cell, angular cell, in all cells, 0.424 0.294 0.188 0.372 OFF Experiment ON-OFF 0.37 ON
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Results of measurement of antineutrino flux from distance, and spectra
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Example of data set in month.
178 useful (ON – OFF) events in days. Relation effect/background (ON-OFF)/OFF = 0.57
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Results of measurements of antineutrino flux from distance
Goodness of fit (1/L2) Goodness of fit (1/L^2) 12% L
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Results of measurements of antineutrino flux from distance
Goodness of fit (1/L^2) 16% L
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ν counting rate dependence on distance from reactor core D А N S
Detector was split into 3 sections along z (~30cm each) Each section has 3 positions – up, middle, down Normalization (efficiency) for central section is a fit parameter Difference in efficiencies of central and 2 other sections are also fit parameters DANSS Preliminary Const/R2 Data are provided M. V. Danilov Perfect agreement with 1/R2 dependence
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Results of measurements of antineutrino flux from distance
Neutrino-4 + DANSS
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Results of measurements of antineutrino flux from distance
Neutrino-4 + DANSS
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Results of measurements of antineutrino flux from distance
Neutrino-4 + DANSS
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GoF = 81%.
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The reactor antineutrino anomaly and sterile neutrino
G. Mention et al., Phys. Rev. D83, , 2011 The reactor antineutrino anomaly and sterile neutrino
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averaged spectrum on all distances
Goodness of fit 13% (Average distance 8.6 m)
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Spectral ratio of experimental prompt signals to expected signals without oscillation
for average spectrum (Average distance 8.6 m) Goodness of fit 13%
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Calculated spectral ratio and experimental spectral ratio
Goodness of fit 78%
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? !
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plot from spectral analysis of Neutrino-4 data
95%
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plot from analysis of distance dependence
95%
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Joint analysis (distance + spectrum)
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Conclusions by results of the current measurements
Dependence of flux of antineutrino is measured for the first time at small distances (6 – 12 m to the reactor center) by means moveable detector. 2. Within the available statistical accuracy reliable deviations from the law 1/L^2 where L – distance to the center of the reactor aren't revealed. The deviation at the level 90% CL isn't significant yet to consider it as reliable deviation. 3. The carried-out analysis within model of a sterile neutrino show a possibility of existence of a sterile neutrino with parameters: However the deviation at the level 90% CL isn't significant yet to declare about observation of sterile neutrino. Analysis of a possible systematics is required also.
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Future plans is the preparation
of new neutrino laboratory at SM-3 reactor in room №170 with two moveable detectors
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Plans: 1. Continuation of measurements on this installation in room №162. 2. Creation of the second neutrino laboratory on the SM-3 reactor with base up to 15 meters in room №170. 3. Two identical detectors, one - stationary on 15 m, the second - mobile. 4. Detectors with PMT from two sides, on 25 PMT from each side. Only 100 PMT. 5. Discrimination of a signal on a form of an impulse (PSD). 6. New scintillator with 0.3%Gd, for suppression of a background of accidental coincidence. ( 3 cubic meters).
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Neutrino laboratory on the SM-3 reactor in room №170
(The aim is the increasing of the accuracy of measurements with factor of 2 or 3) 15 m m SM-3 reactor 1 Scheme of two detectors AS AS (active shielding) AS 2 Fe 10 cm CH2B cm PMT 9354 (25X2)
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Best regards from Dimitrovgrad
А Serebrov1, V Ivochkin1, R Samoilov1, А Fomin1, A Polyushkin1, V Zinoviev1, P Neustroev1,V Golovtsov1, А Chernyj1, О Zherebtsov1, V Martemyanov2, V Tarasenkov2, V Aleshin2, А Petelin3, А Izhutov3, А Тuzov3, S Sazontov3, D Ryazanov4, М Gromov3, V Afanasiev3, М Zaytsev1, 4, М Chaikovskii1 1 Petersburg Nuclear Physics Institute NRC KI, Gatchinа, Russia 2 NRC “Kurchatov institute”, Moscow, Russia 3 JSC “SSC RIAR”, Dimitrovgrad, Russia 4 DETI MEPhI, Dimitrovgrad, Russia
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Studies of background condition by means of gamma and neutron detectors
Gamma detector NaJ Thermal neutron detector He3 PuBe (n) Neutron source Fast neutron detector Calibration procedure
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Fast neutrons are the most danger
Measurement of fast neutron flux near the reactor wall (outside the shielding) during increase reactor power flux of fast neutron 10-3s-1cm-2 Fast neutrons are the most danger
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Distribution of fast neutrons fluxes inside shielding
at Р=90 MWt and at 0 MWt flux of fast neutron 9 x10-5s-1cm-2
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Fast neutrons flux (s-1cm-2)
Thermal and fast neutrons fluxes inside shielding and on top of shielding, Р=90 MWt. Thermal neutrons flux (s-1cm-2) Fast neutrons flux (s-1cm-2) Place of measurment (0.34±0.07) 10-5 (4.4±0.5) 10-5 Inside (17.7±1.2) 10-5 (69±2) 10-5 On the top Shielding factor Кth= 53 Shielding factor Кfast = 16
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near the reactor wall inside the shielding 137Cs 60Co
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Gamma-rays background distribution inside shielding,
Reactor on (Gamma detector NaJ)
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Spectral-integrated dependence
Neutrino-4 NEOS DANSS Biological reactor shielding
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Spectral-integrated dependence
for nuclear power plant NEOS DANSS
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Neutrino-4 7 m DANSS 11.7 m NEOS 24 m
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Background of accidental coincidence. Spectral dependence.
Different distances and power of the reactor. 7.11 метра 10.87 метра
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Background of accidental coincidence, spectral dependence.
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NEOS
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Neutrino-4
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Neutrino-4 7 m DANSS 11.7 m NEOS 24 m prompt energy prompt energy
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Neutrino-4 7 m DANSS 11.7 m NEOS 24 m
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500 m
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Different part of spectrum at the different distance
R/A background Neutrons Muons Soft component of cosmic rays
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Detector active shielding
For multi-section detector
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The detector is based on reaction of the inverse β -decay
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Signal of correlated events
time of arrival of the second impulse prompt signal delayed signal 10 s 100 s time window
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Cosmic rays background
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The effects of atmospheric temperature and pressure on cosmic rays
5% 8% 14%
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Time spectra for different configurations of active shielding (AS)
No AS, Muons 1.54 c-1 = 2,2 = 30 No AS, Neutrons 0.15 c-1 Neutrons 0.011 c-1
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The problem of fast neutrons
Neutron scattering imitate neutrino reaction
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Multi-section model of detector
liquid scintillator PTM Table 1. The probability of double-start events registration in various sections. central section side section corner section average 0.42 0.29 0.19 0.30 Monte-Carlo calculations
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Multi-section antineutrino detector model
The detector consists of 16 sections 22.5 x 22.5 x 50 cm3 with fixed baffles. The baffles are made of acrylic plastic and have specular surface serve to prevent light from leaving the section. Scintillator material is mineral oil (CH2) with addition of Gadolinium 1g per litter.
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General scheme of installation
. 1 – detector of reactor antineutrino, 2 – internal active shielding, 3 – external active shielding (umbrella), 4 – steel and lead passive shielding, 5 – borated polyethylene passive shielding, 6 – moveable platform, 7 – feed screw, 8 – step motor.
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The full-scale detector with liquid scintillator volume of
3 m3 (5x10 sections) is installed already
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Fig. 5. Results of energy calibration.
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Distribution of signals on sections from capture of a neutron gadolinium
Monte Carlo Experiment а – result of Monte Carlo of modeling (the neutron is taken in the middle of section), b– the result received on the sectioned detector (in relative units).
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Distribution of an event of capture of a neutron gadolinium by quantity of the involved sections.
Distribution of the detained signals concerning a cell (3, 3) in which there was a reaction of the inverse beta decay.
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Improvement of the relation a signal/background due to sectioning
S/B =0.1 S/B =0.1 S/B =0.3 S/B =0.3 sectioning S/B =0.6
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Spectra of prompt signals for different distances
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GoF = 48%.
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Spectral ratio of experimental prompt signals to expected without oscillation
for average spectrum Calculated spectral ratio of prompt signals to expected signals without oscillation for different
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