Rudik Dmitry AAP Workshop CEA 2014 1 1 Outline: RED - - PowerPoint PPT Presentation

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Rudik Dmitry AAP Workshop CEA 2014 1 1 Outline: RED - - PowerPoint PPT Presentation

NATIONAL RESEARCH NUCLEAR UNIVERSITY MEPhI (Moscow Engineering Physics Institute) Laboratory for Experimental Nuclear Physics http://enpl.mephi.ru/ The RED-100 Search for elastic coherent neutrino scattering off atomic nuclei at the


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The RED-100 Search for elastic coherent neutrino scattering off atomic nuclei at the Kalininskaya Nuclear Power Plant

Rudik Dmitry

AAP Workshop CEA 2014 NATIONAL RESEARCH NUCLEAR UNIVERSITY MEPhI (Moscow Engineering Physics Institute) Laboratory for Experimental Nuclear Physics

http://enpl.mephi.ru/

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Outline:

 RED Collaboration  RED-1 & obtained results  RED-100 & Kalininskaya Power Plant  Conclusion

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2010

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D.Sc. -2 PhDs – 10 Faculty - 12 PhD students – 6 Students – 10

LENP LENP

2011

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10-44 10-43 10-42 10-41 10-40 10-39 2 4 6 8 10 C r

  • s

s S e c t i

  • n

[ c m

2

] Neutrino Energy [MeV]

Elastic Scattering off Ar Proton Inverse Beta Decay

σ elastic = GF

2

4 π N2 Eν

2

≈0.4× 10−44cm2 A2 Eν(MeV)2

Erecoil ⩽ 716 eV Eν

2(MeV)

A

Large cross-section Small recoil energies

θ ν , k ν , k ’

q

N e u t r a l c u r r e n t

+ + + +

θ ν , k ν , k ’

q

N e u t r a l c u r r e n t

+ + + + + + + +

Coherent neutrino scattering off heavy nuclei

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IEEE TRANSACTIONS ON NUCLEAR SCIENCE, VOL. 50, NO. 5, OCTOBER 2003

  • P. S. Barbeau, J. I. Collar, J. Miyamoto, and I. Shipsey

Recoil spectra from reactor e-antineutrino

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C.Hagmann and A.Bernstein. Two-phase emission detector for measuring coherent neutrino-nucleus scattering, IEEE Trans. Nucl. Sci. 51(2004)2151-2155.

LAr detector @ LLNL

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8 Болоздыня 24.11.2011

7 FEU-181, MgF2

LXe RED-1 & Research reactor of MEPhI

arXiv:1212.1938

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2.5 MW Research reactor IRT MEPhI

1 – RED-1 2 – Fe/Al filter 3 – horizontal neutron channel GEK10 4 – starting point of MCNP simulations 5 – cooling water pool 6 – active zone 7 – heavy concrete shielding

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10 1 – detector RED-1; 2, 3 - shield 10 cm lead & 10 cm borated polyethylene; 4 — lead slice 5 cm; 5 polyethylene slice - 5 cm; 6 - paraffjn; 7,8 – fjlter 30 cm Fe & 70 cm Al; 9 — reactor's concrete shield. Specifjc ionization yield for the nuclear recoil with energy < 1 keV isn't known. Its obtainig is the main goal of our experiment at the MEPhI reactor. Neutron total cross section of 27Al and of 56Fe (upper plot) and simulated neutron beam spectra before and after passing the filter (bottom plot).

arXiv:1212.1938

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11 Distribution of EL (S2) signals generated by single emitted electrons (green). Maximum of the Gauss fit is 15 ± 5 photoelectrons. Poisson distribution for 10 and 15 expectations are shown in pink and violet, respectively. Typical gamma event in RED-1

Detection of Single Electrons

A.A. Burenkov et al Phys.Atom.Nucl. 72 (2009) 653-661,

  • Yad. Fiz. 72 (2009) 693-701

Doi: 10.1134/S1063778809040103

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12 12

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Obtained results

Experimental data for the ionization yield of LXe for electron recoils and theoretical predictions

D.Yu. Akimov et al 2014 JINST 9 P11014 doi:10.1088/1748-0221/9/11/P11014

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Source Energy, keV Ionization yield, e-/keV

37Ar

2.82 48.3 ± 5.7 (syst.)

241Am, Np

Lβ1 17.75 44.9 ± 2.7 (stat.) +

3.3 (syst.) – 5.1 (syst.) 241Am, esc.

peak (59.5- 29.5 keV) 30 47.8 ± 0.7 (stat.) +

3.3 (syst.) – 3.4 (syst.) 129Xe

40 49.0 ± 0.4(stat.) ± 1.7 (syst.)

83mKr

41.5 43.7 ± 0.1 (stat.) ± 2.8 (syst.)

241Am

59.5 49.5 ± 0.1(stat.) ± 3.4 (syst.)

131Xe

80 55.6 ± 0.8 (stat.) +

1.6 (syst.) – 1.9 (syst.) 137Cs

662 63.0 ± 0.2 (stat.) +

3.2 (syst.) – 3.8 (syst.)

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USA Kalininskaya NPP

1 m 0 . 5 m

H A M A M A T S U R 8 7 7 8

RED-100

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15 Titanium Warm vessel Tefmon Drift cage Titanium Cold vessel Array of 19 PMTs in Copper holder Thermosyphon Cold Head Copper T

  • screen

1m 68 cm 64 cm

RED-100

Material Mass, kg Copper 310 Tefmon 82 PMT R11410 38 pcs Titanium 221 Array of 19 PMTs in Copper holder Hamamatsu R11410-20 15

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1 0 0 2 0 0 3 0 0 4 0 0 5 0 0 6 0 0 7 0 0 8 0 0 9 0 0 1 0 0 0 1 1 0 0 1 2 0 0 1 3 0 0 1 4 0 0 1 5 0 0 1 6 0 0 1 7 0 0 1 8 0 0 1 9 0 0 1 1 0 1 0 0 1 0 0 0 1 0 0 0 0 O f f i c e ( 2 7 . 0 9 . 2 0 0 6 ) R o o m A 3 3 6 ( 2 9 . 0 9 . 2 0 0 6 )

γbackground under the reactor γbackground in the lab Energy, keV d N \ d E , c

  • u

n t s / k e V / k g / s

Kalininskaya Nuclear Power Plant (Udomlya)

GEMMA

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17

Signal/Noise A: fSEE=100Hz B: fSEE=10Hz C: Signal CR (>2 e) = 433/day/100 kg LXe

СR (E>1,8 MeV) = 27000/day/100kgLXe

Signal/Background A: detector components B: neutrons C: Signal

Kalininskaya NPP facility: Фantineutrino = 1.35*1013 cm-2s-1

arXiv:1212.1938

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18 Neutrino Spectra from fusions

Monitoring nuclear reactors

Detector response Antineutrino flux evolution Daily power monitoring

LWR, 3GWt, L = 19m

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19

Conclusion

  • Emission two-phase detectors are much promising

technology to search for the Coherent Neutrino Scattering (CNS) effect

  • CNS is interesting for fundamental Physics and for non-

proliferation applications

  • Capability to measure weak ionization from nuclear recoils

below 1 keV energies is a key element toward the observation

  • f CNS

 Obtained results by RED-1 of low energy recoils region show

an ability of such detectors to search for CNS effect

  • RED-100 experimental installation is under development for
  • bservation of CNS and for development of a highly sensitive

method of NPP monitoring

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Thank you for your attention!

Our contacts:

  • http://enpl.mephi.ru - our website
  • E-mails
  • yefremen@utk.edu - Dr. Yuri Efremenko
  • AIBolozdynya@mephi.ru - Dr. Alexander Bolozdynya
  • akimov_d@me.com - Dmitry Akimov
  • Rudik.dmitry@mail.ru - my e-mail
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Backup

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16.12.14 Болоздыня

Electronics: RUN2013

LXe MEPhI 2014

Signals from PMTs Fast preamplifiers High sensitivity channel Low sensitivity channel 8-channel Phillips Scientific 772

A remote control switch. 0.5 or 5 gain possibility

Struck SIS3350 12-bit (2 ns sampling) CAEN V1720 12-bit (4 ns sampling)

From a fraction of a SPE to ~105 SPE!

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16.12.14 Болоздыня

Calibration sources

LXe MEPhI 2014

Energy, keV 2.82 13.9 17.2 30 39.6 41.5 59.5 80.2 662 Isotope

37Ar 241Am 241Am 241Am 129Xe 83mKr 241Am 131Xe 137Cs

Description EC, Auger gamma gamma escape peak n-gamma IC, gamma, Auger gamma n-gamma gamma RUN2009 – + + + – + + – – RUN2013 + – – – + + – + +

Table of energy lines and corresponding radioactive sources

83mKr line was used as a reference point to combine results

  • f both datasets
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16.12.14 Болоздыня

Data analysis: 37Ar

LXe MEPhI 2014

Distribution of S2 signal areas of 37Ar and 83mKr events; red - events from the 83mKr runs, blue – events from 37Ar runs, green – events from the runs with both 37Ar and 83mKr in the detector (without lifetime correction).

The evaluated from 37Ar data free electron lifetime is 16 ± 5 μs. Weighted average of krypton to argon ratio is

13.3 ± 1.3

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16.12.14 Болоздыня

Ionization yield: Wi

LXe MEPhI 2014 Wi = 15.6 ± 0.3 eV (for MeV 207Bi electrons and γ)

  • T. Takahashi, S. Konno, T. Hamada et al., Phys. Rev. A12 (1975) 1771,

Average energy expended per ion pair in liquid xenon Wi = 16.5 ± 0.8 eV (for 122 keV 57Co γ)

  • M. Horn, V. A. Belov, D. Yu. Akimov et al., Phys. Lett. B705 (2011) 471,

Nuclear recoil scintillation and ionisation yields in liquid xenon from ZEPLIN-III data Wi = 14.27 ± 0.30 eV ← (1 + 0.06) * W = 13.46 ± 0.29 eV

  • T. Shutt, C.E. Dahl, J. Kwong et al., NIM A579 (2007) 451,

Performance and fundamental processes at low energy in a two-phase liquid xenon dark matter detector Wi = 13.6 ± 0.2 eV

  • I. M. Obodovskii and S. G. Pokachalov, Sov. J. Low Temp. Phys. 5 (1979) 393,

Average ion pair formation energy in liquid and solid xenon Wi = 14.84 eV ← (1 + 0.06) * W = 14 eV

  • E. Aprile J. Angle, F. Arneodo et al., Astropart. Phys. 34 (2011) 679,

Design and performance of the XENON10 dark matter experiment

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Spallation Neutron Source (ORNL)

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I n t e r f a c e L N D e w a r

Ground shielding 40 m from target neutrino 10 m below ground level

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Signal/Noise A: fSEE=100Hz B: fSEE=10Hz C: Signal CR (>3 phe) = 1470/year/100 kg LXe Signal/Background A: Neutrons from cosmic rays B: Components of RED100 C: Neutrons from SNS D: Signal

RED-100 @ 40 m from the SNS target

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  • V

V ( z ) z p d N / d p z z e e e

Quasi-free electron emission from nonpolar dielectrics

  • V

V ( z ) z e

1

V ( b )

V 1( z )=V 0−eF1z+eA1,z<0 V 2(z)=−eF2 z+eA 2,z>0

A1,2=−e( ε1−ε 2)/[4 ε1,2(z+ξz/|z|)(ε1+ε 2)]