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150 Nd activities at TUM. V. Lazarev 1 , E. Nolte 1 , L. Oberauer 1 , F. Pröbst 2 1 -Technische Universität München, E15 2 -Max Planck-Institut für Physik , München. with help of J. Doncev 2 , V. Kochurichin 3 , L. Nagorna 4 , D. Kovalev 5 , S. Schönert 6 , M. Stark 1 - PowerPoint PPT Presentation
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21. October 2004 IDEA DBD Meeting, Heidelberg
150Nd activities at TUM V. Lazarev1, E. Nolte1, L. Oberauer1, F. Pröbst2
1 - Technische Universität München, E152 - Max Planck-Institut für Physik, München
with help of
J. Doncev2, V. Kochurichin3, L. Nagorna4, D. Kovalev5, S. Schönert6, M. Stark1
3 - General Physics Institute, Coherent and Nonlinear Optics Department, Russia4 - Institute for Single Crystals, Ukraine5 - Technische Universität München, E166 - MPI, Heidelberg, Germany
21. October 2004 IDEA DBD Meeting, Heidelberg
emitters
Isotope Q, keV T 2, 1019 a
T 0 for <m>=50 meV, 1026 a
(T2/ T0
, 10-7)
48Ca 4271 4 4.2 1.2 12.7
(0.33) 35 (0.1) 10 (0.4)
76Ge 2040 1 13 10 6.8 (19) 71 (2) 56 (2.3) 9.3 (14) 12.8 (10)
14.4 (9)
82Se 2995 6 9.2 1.0 2.3 (4) 9.6 (1) 22 (0.4) 2.4 (4) 3.2 (3) 6 (1.5)
100Mo 3034 6 0.8 0.06 5 (0.2) 1.2 (0.7) 16
(0.05)
116Cd 2802 4 3.2 0.3 1.9 (1.7) 3.1 (1) 18.8 (0.2)
130Te 2533 4 270 10 0.6
(450) 23 (12)
2.8 (100)
2 (135) 3.6 (75) 3.4 (80)
136Xe 2479 8 >81 48.4 8.8 21.2 7.2
150Nd 3367 2 0.7 + 1.2 – 0.3 0.1 (7) 0.2 (3.5)
A. Staudt A. Faessler
150Nd:• the shortest half-time for neutrinoless 0 decay• the second largest Q-value• low 2 background
21. October 2004 IDEA DBD Meeting, Heidelberg
Tungstates and scintillation
Almost all tungstates scintillate.The best known scintillators are:CdWO4, PbWO4, CaWO4
The reason is the structure of WO4
From: Williams R.T., Y.C. Zhang, Y. Abraham, and N.A.W. HolzwarthElectronic structure of pure and defective PbWO4, CaWO4, and CdWO4
Invited paper presented by R.T. Williams at the SCINT99 conference in Moscow, Aug. 1999
21. October 2004 IDEA DBD Meeting, Heidelberg
Crystal scintillators• Tungstates are often scintillators: CaWO4, CdWO4, PbWO4
• Measurements with CdWO4 are done with low background: 0.03 counts/(keV kg a) (Danevich F.A. et al. Phys. Rev. C62:044501 (2000))• Crystals of CaWO4 can have good resolution: 5% at 1332 keV (F. Pröbst)
Crystal of Nd2(WO4)3 is probably a scintillator
Detector resolution could be %31332
05.0 Q
keV
1%64.5503
280 44
M
kg
T
ameVm With |M0|2 from Staudt,
21. October 2004 IDEA DBD Meeting, Heidelberg
Current state of the investigationWe need highly enriched neodymium (Russia!):
1%852005
45 44
M
kg
T
ameVm
• A process of Nd2(WO4)3 growing was investigated. • Sample crystals were grown using Czochralski method (V. Kochurichin, Moscow).
21. October 2004 IDEA DBD Meeting, Heidelberg
Crystals
Successful crystals of CaWO4
21. October 2004 IDEA DBD Meeting, Heidelberg
Current state of the investigationWe need highly enriched neodymium (Russia!):
1%852005
45 44
M
kg
T
ameVm
• A process of Nd2(WO4)3 growing was investigated. • Sample crystals were grown using Czochralski method (V. Kochurichin, Moscow). • 3 small crystals (about 1 cm3 each) were delivered to Munich
21. October 2004 IDEA DBD Meeting, Heidelberg
Scintillation
dark box
to electronic
Crystal
PMT, XP3461B
standard source
90Sr, 137Cs
60Co
Jelena Doncev, MPI, München
No clear result!
21. October 2004 IDEA DBD Meeting, Heidelberg
Spectral characteristics
Nd2(WO4)3 crystal
grid
focusing mirror focusing mirror CCD camera Prinston Instruments GmbH cooled with liquid N2
Monochromator: Special Pro-250, Acton Research Corporation
Sensitivity: 400 (300) – 1000 nm
D. Kovalev, TU München, E16
21. October 2004 IDEA DBD Meeting, Heidelberg
Current state of the investigationWe need highly enriched neodymium (Russia!):
1%852005
45 44
M
kg
T
ameVm
• A process of Nd2(WO4)3 growing was investigated. • Sample crystals were grown using Czochralski method (V. Kochurichin, Moscow). • 3 small crystals (about 1 cm3 each) were delivered to Munich• The crystals showed no scintillation (J. Doncev, MPI, D. Kovalev, TUM, E16)• A powder of other compositions (e.g. LiNd WO4) showed no roentgen-luminescence (L. Nagorna, Ukraine)
21. October 2004 IDEA DBD Meeting, Heidelberg
The choice of a detector
Direct counting Other
150Nd is within detector 150Nd is outside detector
Electron hole pairs(Semiconductors)
Production of photonsand photoelectrons
(Scintillators)
Production of phonons(Cryodetectors)
Crystal scintillators
Liquidscintillators
Production of phonons(Cryodetectors)
21. October 2004 IDEA DBD Meeting, Heidelberg
Cryogenic detectors
Heat capacity of an insulator
3
D
Tc
Heat capacity of a ferromagnet
If there is an energy splitting
2
2
1 T
T
e
eTc
Energy resolution
)(2 TcTkE B
In case of thermalization
Temperature increase
t
eTc
EtT
)()(
Low heat capacity is necessary!
2
3
A
Tkc B
21. October 2004 IDEA DBD Meeting, Heidelberg
• Particle or light interaction with absorber
• High frequency phonons are produced
• Phonons become ballistic and fill the crystal homogeneously
• In the Al-phonon collector those phonons break up quasiparticles
• Quasi particles diffuse to the Ir/Au-superconducting thermometer and heat it up
• Resistance of the film changes and the resistance of the thermometer
Al-phonon-collector
Ir/Au-thermometer
Cryodetectors at TUM
21. October 2004 IDEA DBD Meeting, Heidelberg
• Particle or light interaction with absorber
• High frequency phonons are produced
• Phonons become ballistic and fill the crystal homogeneously
• In the Al-phonon collector those phonons break up quasiparticles
• Quasi particles diffuse to the Ir/Au-superconducting thermometer and heat it up
• Resistance of the film changes and the resistance of the thermometer
Al-phonon-collector
Ir/Au-thermometer
Cryodetectors at TUM
21. October 2004 IDEA DBD Meeting, Heidelberg
• Particle or light interaction with absorber
• High frequency phonons are produced
• Phonons become ballistic and fill the crystal homogeneously
• In the Al-phonon collector those phonons break up quasiparticles
• Quasi particles diffuse to the Ir/Au-superconducting thermometer and heat it up
• Resistance of the film changes and the resistance of the thermometer
Al-phonon-collector
Ir/Au-thermometer
Cryodetectors at TUM
21. October 2004 IDEA DBD Meeting, Heidelberg
• Particle or light interaction with absorber
• High frequency phonons are produced
• Phonons become ballistic and fill the crystal homogeneously
• In the Al-phonon collector those phonons break up quasiparticles
• Quasi particles diffuse to the Ir/Au-superconducting thermometer and heat it up
• Resistance of the film changes and the resistance of the thermometer
Ecooper-pairs Eprox
aluminum Ir/Au
quasiparticles
phonon
Cryodetectors at TUM
21. October 2004 IDEA DBD Meeting, Heidelberg
• Particle or light interaction with absorber
• High frequency phonons are produced
• Phonons become ballistic and fill the crystal homogeneously
• In the Al-phonon collector those phonons break up quasiparticles
• Quasi particles diffuse to the Ir/Au-superconducting thermometer and heat it up
• Resistance of the film changes and the resistance of the thermometer
Ecooper-pairs Eprox
aluminum Ir/Au
quasiparticles
Cryodetectors at TUM
21. October 2004 IDEA DBD Meeting, Heidelberg
• Particle or light interaction with absorber
• High frequency phonons are produced
• Phonons become ballistic and fill the crystal homogeneously
• In the Al-phonon collector those phonons break up quasiparticles
• Quasi particles diffuse to the Ir/Au-superconducting thermometer and heat it up
• Resistance of the film changes -> this is the signal
R
T
Cryodetectors at TUM
21. October 2004 IDEA DBD Meeting, Heidelberg
Neodymium cooling
NdGaO3
Thermostat
M. Stark,E15, TUM
• Ir/Au thermometer was glued on the NdGaO3 crystal• Only signals from the thermo- meter were detected
• Ir/Au thermometer was sputtered on the NdGaO3 crystal• The results are not available yet
21. October 2004 IDEA DBD Meeting, Heidelberg
Liquid scintillators
A scintillator like CTF could be used
PMTs cover about 20% of the solid angle
penE
E %1323.2
where npe – number of photoelectrons
The energy resolution for CTF
Photoelectron yield of the CTF with100 PMT
MeV
ronsphotoelect300
21. October 2004 IDEA DBD Meeting, Heidelberg
Liquid scintillatorsWith 400 PMT the energy resolution
keVEE
E160%,8.4
Background at 3.3 MeV
akeVkgB
1109.2 5
Now it is possible to solve about 1 %0 of Nd (S. Schönert, MPI, Heidelberg)
21. October 2004 IDEA DBD Meeting, Heidelberg
Local tasksIf we assume that everything is perfect and not additional problem arises
1. Preliminary investigation with natural Nd
4
3
44
4 5
0 1051
1601109.2
%1%64.5260
CTFM
kg
T
a
keV
E
akeVkg
BmeVm
This is sufficient to prove the results of Klapdor-Kleingrothaus, m=400 meV
2. The second step with enriched Nd
4
3
44
4 5
0 1053
1601109.2
%1%8550
CTFM
kg
T
a
keV
E
akeVkg
BmeVm
This is sufficient to prove the inverse hierarchy
21. October 2004 IDEA DBD Meeting, Heidelberg
Summary
• 150Nd is one of the most interesting candidates to detect a neutrinoless double beta decay• There is no established method to measure this decay• Estimations show that it could be possible to build a scintillation detector. However, till now no scintillator with Nd was found. (Maybe because of the properties of Nd).• It is possible to cool Nd-crystal at least down to 60 mK. However, no phonon signal could be measured• A liquid scnitillator with dissolved 150Nd is the most promising idea at the moment