f. piquemal modane underground laboratory (cnrs/ni2p3 and cea/irfu) tpc 2014 paris decembre, 15-17...
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Double beta decay experiments
F. Piquemal
Modane Underground Laboratory (CNRS/NI2P3 and CEA/Irfu)
TPC 2014 Paris Decembre, 15-17 2014
Many thanks to : K. Zuber, S. Schoenert, K. Inoue, A. Giuliani, S. Elliot, M. Chen, M. Nomachi, N. Ishihara. H.J. Kim, F. Danevich, L. Winslow
Nature of neutrino Dirac or Majorana
Neutrino mass hierarchy Right-handed current interaction
CP violation in leptonic sector
Search of Supersymetry and new particles
Double beta decay : physics case
sum electron energy / Q Mass vs Right-Handed Current mechanism
Angular distribution
MM MMRHC
Ee1 – Ee2 distribution
RHC
Decay to Excited States
(A,Z) (A, Z+2) + 2 e- + 1,2 g
1 or 2 additonnal g-rays
Identification of daugther nucleus : Xe Ba++ + 2 e-
(A,Z) (A,Z+2) + 2 e-
Double beta decay observables
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Dueck et al. Phys,. Rev. D 83 113010(2011)
Isotope choice
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Nucleus Existing method R&D48Ca Laser separation,
gazeous diffusion76Ge Centrifugation
82Se Centrifugation
96Zr Laser separation
100Mo Centrifugation
116Cd Centrifugation
130Te Centrifugation
136Xe Centrifugation
150Nd Centrifugation, Laser
R&D in KAERI (Korea) for 48Ca enrichment by laser
R&D in Russia for150Nd enrichment by centrifugation
R&D in France for150Nd enrichment by laser
Isotope enrichment
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T0
2/1
eA
M . t
NBckg . DE(y)
WITH Background
e :efficiency, M: Mass, t: time, Nbckg: Background events, DE: energie resolution, A: isotope mass
Other sources of background: Muons (underground labs) g from ( (n,g) reactions , m
bremstrahlung Muon spallation products a emitters from bulk or surface
contaminations for calorimeters (2 ) bb n if modest energy resolution
208Tl (2.6 MeV g )
214Bi (and radon)
208Tl (and thoron)
E (M
eV)
40K, 60Co,…
Different strategies are possible to minimize the background
Transistion energy Q
bb
Background originsNatural radioactivity
Backgrounds
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Calorimeter
Tracko-calo82Se (150Nd,48Ca)NBckg , isotopes
Pixellized CdZnTe116Cde, NBckd
TPC136Xe, 150Nde, NBckd
Ge diode 76Gee, DE
Bolometers130Te,82Se,100Mo
e, DELiquid Xe
136Xee,M,(Nbckd)
Scintillator136Xe, ,48Ca,
150Nd, 100Moe, M
GERDAMAJORANA
CUORELUCIFERLumineuAmore
EXO
KamLAND-ZenCANDLES
SNO+BorexinoCdWO4AMoRE
SuperNEMO
COBRA
MTDEXO-gasNEXT
Tracker
Next generation of experiments
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100 – 1000 cts/yr/ton
1 – 10 cts/yr/ton
0.1 – 1 cts/yr/ton
Isotopemass
~ 10 kg 2012
~ 1000 kg
Required background levelin the ROI
|mee
|
S T Petcov 2009 J. Phys.: Conf. Ser. 173 012025
~ 100 kg 2015
Next generation will use ≥ 100 kg (started with Xe experiments)
Improvements of background level needed
(200 – 400kg 136Xe)
Goal of the next generation
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In case of (0 ) bb n through light neutrino exchange
10 kg: T1/2 > 1024-1025 years 100 kg: T1/2 > 1026-1027 years :
SuperNEMO ConstructionNEXT R&DEXO R&DMTD (DCBA) R&DCOBRA R&D
Tracking experiments
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[2.8 – 3.2] MeV 18 observed events, 16.4 ± 1.3 expected
100Mo T1/2 ( 0bb n) > 1.0 1024 y (90% C.L.)
<mn> < 0.31– 0.79 eV
event
E1+E2= 2088 keV t= 0.22 ns(vertex) = 2.1 mm
E1
E2
e-
e-
Unique featureMeasurement of all kinematic parameters: individual energies and angular distribution
Tracking detector: drift chambers (6180 Geiger cells) t = 5 mm, z = 1 cm ( vertex ) Calorimeter (1940 plastic scintillators and PMTs) Energy Resolution FWHM=8 % (3 MeV) Identification e-,e+, Very high efficiency for background rejection Background level @ Qbb [2.8 – 3.2 MeV] : 1.2 10-3 cts/keV/kg/y Multi-isotope (7 measured at the same time) Running at Modane underground laboratory (2003 - 2011)
Measurement of 7 isotopes (2 ) bb n half-lifesExcited states, Majoron limits for (0 )bb n
NEMO3
TPC 2014 (APC Paris) 11
A module 20 modules
Demonstrator module
20 Modules
Source : 82Se 7 kg 100 kg
Drift chambers for tracking 2 0000 40 000
Electron calorimeter 500 10 000
g veto (up and down) 100 2 000
T1/2 sensitivity 6.6 1024 y(No background)
1. 1026 y
<m> sensitivity 200 – 400 meV 40 – 100 meV
Located in LSM extension
SuperNEMO
F. Piquemal
Calorimeter
DE/E < 4% @ 3 MeV(NEMO3 8.6% at 3MeV)
Source
214Bi < 10 mBq/kg (NEMO3 100 mBq/kg)208Tl < 2 mBq/kg(NEMO3 100 mBq/k)
Tracker
3.7 m long (NEMO3 2.7 m) t = 5 mm, z = 1 cm Radon < 0.15 mBq/m3
(NEMO3 5 mBq/m3)Wiring robot
Global efficiency : 30 % (NEMO3 8%)
Objective: to reach the background level for 100 kg to perform a no background experiment with 7 kg isotope of 82Se in 2 yr
SuperNEMO
- Scintillators production and 8’’ Hamamatsu PMT’s in production- FE digitizer boards OK, control and trigger boards under development- Blocks, wall design and technical tests OK construction in progress 1st wall @ LSM in 2014
- Automated drift cells production ongoing with the wiring robot- First 1 / 4 tracker C0 tested for radon emanation and cells propulation- C0 commissioning at see-level and underground @LSM in 2014
- 5.5 kg of 82Se , 4.5 kg already purified. Purchase of 1.5 kg in progress- Source materials (glue, films,…) under HPGE and BiPO selection processes- Calibration sources deployment system and LED survey system under test
Calo
rimet
erTr
acke
rSo
urce
SuperNEMO Demonstrator status
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Ultra low background detector Modular detector with 3 main components :
Central source foil frame : 7 kg of isotope Tracking : 2 000 drift chambers Calorimeter : 712 scintillators+ PMTs
Shielded by iron (300 tons) and water Construction in progress Installation and commissioning at Modane
Underground Laboratory 2015 – 2016 Data taking 2016
Source
tracker
Calorimeter
SuperNEMO demonstrator module
No background expected for 2 years of data. 7 kg 82Se T1/2 > 6.6 1024 y <mn> < 0.16 – 0.44 eV
Use large amount of CdZnTe Semiconductor Detectors
K. Zuber, Phys. Lett. B 519,1 (2001)
• Source = detector
• Semiconductor (Good energy resolution, clean)
• Tracking/Pixelisation („Solid state TPC“)
• Modular design (Coincidences)
• Focus on 116Cd
• Room temperature
COBRACobra
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Objective : Massive background reduction by particle identification
Bi-214 =Time coincidence of both
alpha electron
alphaelectron
55 μm pixel real event
Real event!
COBRA
Current spectrum (black), 12.73 kg*daysBackground at 2813 keV about 1 ct/keV/kg/yr
Currently ongoing upgrade:- 64 detectors (in hand) 32 running at LNGS- Pulse shape information - rejection of surface events
116Cd peak region
Cobra
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Chamber cell : the same as DCBA-T3, Source plate: 80 m2/moduleThickness: 40 mg/cm2, Source weight: 32 kg/module
MTD (Magnetic Tracking Detector: temporary name) following of DCBA
Expected Energy Resolution 3.4% at Qbb for 150Nd
Multi-isotope 150Nd, 100Mo, 82SeSeveral modules to reach <mn> 50 meV
Magnetic Tracking Detector (DCBA)
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GERDA II In progressCUORE In progress KamLAND-Zen In progress CANDLES Data taking SNO+ In preparationMAJORANA Completion of R&DLUCIFER R&DZnMoO4 R&DAmore R&DCdWO4 R&D
Calorimetric experiments
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L. Winslow Neutrino 2014
Ge diodes
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Ge detectors in liquid nitrogen installed @ LNGS
GERDA II : Ge diodes
Phase I: 14.6 kg of enriched detectors
Background level after Pulse shape discrimination0.01 cts/(keV.kg.yr).
Exposure 21.6 kg.yr
GERDA: T1/2 > 2.1 1025 yr (90%CL)
GERDA+ IGEX. HM T1/2 > 3.0 1025 yr <mn> < 0.2 – 0.4 eV
Integration of the elements of GERDA phase II40 kg of enriched Ge detectors
- First deployment of the liquid argon scintillation readout. - First pilot string will be deployed together with the LAr scintillation read out. - Deployment of the full array of enriched Ge detectors early next year.Phase II is designed to reach T1/2 > 1026 years.
GERDA II : Ge diodes
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TPC 2014 (APC Paris) 22
Improvement of the radiopurity of the materials, Pulse shape– Cryostat 1 (3 strings enrGe & 4 strings natGe) (Fall 2013)– Cryostat 2 (up to 7 strings enrGe) (Fall 2014)
Final design of demonstrator 30 kg of 76Ge and 10 kg of natGe
Majorana : Ge diodes
F. Piquemal
- Purification of liquid scintillator to remove 110mAg- Improvement of spallation cut- Improvement of fiducial volume selection
KamLAND-ZEN
(Kamioka)
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KamLAND-ZEN prospectives
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CUORE: bolometers
CUORE-0 has validated the energy resolutionAnd background results are encouraging
All the towers are assembled
Cryostat cooled down to 6 mK with 470 kg of Cu
Presently, cooling with 8 bolometers for test
CUORE-0
741 kg of TeO2 bolometers (206 kg of 130Te) @ LNGS
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CANDLES III @ Kamioka
96 CaF2: 305kg (57 g of 48Ca) + liquid scintillator
Measurement started in June 2011.
CANDLES III
Cooling system(~0 ) (october 2014)℃
Coils to compensate magnetic filed
Improvement of energy resolution 4% (FWHM) @ Qbb
Enrichment of 48Ca (2%)
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NatTe dissolved in liquid scintillator (0.3% corresponding to 800 kg of 130Te
5 years of data
SNO+
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Heat energy [keV] Heat energy [keV]
Ligh
t/H
eat [
keV/
keV]
Shap
e pa
ram
eter
Example of b/a rejection with a 5 g detector
Scintillating bolometers
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Scintillating bolometers to recognize the -induced background thanks to the readout of the scintillation light
Array of 36÷44 enriched (95%) Zn82Se crystals.
Expected background in the ROI (2995 keV) is 36 10-3 c/keV/kg/y
Zn82Se crystal (Ø=45mm, h= 55 mm)
W=483 g
Reflecting Foil
PTFE supports
Bolometric Light DetectorGe crystal
Energy resolution 10 keV FWHM
LUCIFER
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Calibration aboveground
spectrum
Two enriched crystals of 60 g each obtained Excellent performance aboveground (CSNSM, Orsay) No difference with respect to natural crystals
nderground tests of a few large mass enriched crystals (foreseen within June 2015)
If radiopurity is confirmed:
Systematic production of 40 crystals containing 7 kg of 100Mo (MoU INFN+IN2P3+ITEP)
Start-up of LUCINEU project (LUCIFER+LUMINEU)
Cool down of this 40 crystal array during 2016 in LNGS and/or LSM (depending on cryostat availability)
LUMINEU
40Ca100MoO4 bolometers 15 keV FWHM, Eff = 0.8
(Advanced Mo-based Rare process Experiment)
AMoRE Pilot, 20155 bolometers de CaMoO 1,5 kg
StageStart
(run, yr)
Background
(yr/keV/kg)
Sensitivity limT1/2 (yr) m (eV)
AMoRE pilot
Jan. 2015 (1) 0.01 ~1.5x1024 <0.3 –
0.9
AMoRE 10 Sep. 2016 (3) 0.002 ~2x1025 0.08 -
0.22AMoRE
200Jan. 2019
(5) 0.0002 ~41026 0.016 - 0.047
AMORE
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76Ge
82Se
136Xe
100Mo
116Cd
130Te
Nat(150)Nd
Nat(48)Ca
GERDAMAJORANA
KamLAND-ZenEXO - NEXONEXT
LumineuAMoRE
SuperNEMOLUCIFER
COBRACdWO4
CUORE
SNO+Borexino
CANDLES
48Ca
150Nd
CANDLESSuperNEMOAMoRE
SNO+SuperNEMOMTDBorexino
A dream ?
Studied isotopes
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Experimental limit (90%CL)
EXO-200KamLAND-Zen
CUORE
Solotvina
NEMO3
NEMO3
NEMO3CANDLES
GERDA
Half-life to reach for <mn> = 50 meV
Present experiments at the level of T1/2 > 1024 – 1025 years<mn> < 0.15 – 0.5 eV
Several experiments at 100 kg are needed to understand backgrounds and determine the best isotope and technique for higher mass
Sensitivity : T1/2 > 1026 – 1027 years<mn> < 0.05 – 0.1 eV
Starting to test of the inverted hierarchy scenario
2015 - 2016 : starting of GERDA II, Majorana, SuperNEMO, SNO+, CUORE, scintilating bolometers
Still a long way to reduce the background.
In case of signal a tracking experiment will be needed to confirm it
Summary