double beta decay, neutrino physics and something else 1 1.the birth of double beta decay 2.from low...
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Double beta decay, neutrino physics and something else
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1. The birth of double beta decay2. From low energy nuclear physics to neutrino mass and
properties3. The physics of rare events 4. Experimental approaches and difficulties5. Present experimental status6. The future7. The nightmare of nuclear matrix elements 8. Something else9. Conclusions
Benasque March 19,2015 Ettore Fiorini
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2Benasque March 19,2015 Ettore Fiorini
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Double beta decays
1935 M.Goeppert-Mayer, P.R. 48 (1935) 512 T>1020
Majorana, Nuovo Cimento 14 (1937) 171 Symmetric Theory of Electron and Positron G. Racah, Nuovo Cimento 14 (1937) 322
W.H. Furry Lepton number nonconservation
1967: 130Te, Geochemical Ogata and Takaoka, Kirsten et
1987: 82Se, Direct counting Moe et al .1987 : Source=detector 48Ca, 76Ge
3Ettore Fiorini Benasque March 19,2015
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1. (A,Z) => (A,Z+2) + 2 e- + 2 e
Two neutrino double beta decay Allowed by the standard model Found in eleven nuclei ( 130Xe is new!) to ground state and in two
to excited state
2. (A,Z) => (A,Z+2) + 2 e- + ( …2,3 ) Emission of a massless Goldston boson named Majoron (Gelmini and Roncadelli)
3. (A,Z) => (A,Z+2) + 2 e-
Neutrinoless double beta decay. The two electrons share the total transition energy E1 + E2 => E => a peak should appear in the sum spectrum of the two electrons
Other possible “L=2” decays- Double positron decay => + + - Positron decay + Electron Capture => EC- + - Double electron capture => EC-EC
4Benasque March 19,2015 Ettore Fiorini
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Two neutrino and neutrinoless double beta decay
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Measurement of the CP phase in the decay
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e-
e-
Direct experiments
Source detectors Source = detector
Geochemical experiments82Se = > 82Kr, 96Zr = > 96Mo, 128Te = > 128Xe , 130Te = > 130TeRadiochemical experiments 238U = > 238Pu (non confirmed)
How to search for decay
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Many types of detectors
Experimental challenges
• Cloud chambers
• Emulsions?
• Bubble chambers ? (yes for Dark Matter)
• Scintillators
• Double state liquids
• Time projectrion chambers
• Tracking and imagining devices
• Single atom counters 136Xe => 136Ba
• Bolometers
• Hybrid devices
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A first source = detector experiment
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RARE events One of the main problem => background
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Cosmic rays => underground physics
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Where to go ?
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The Jin Ping Laboratory (700 m.w.e)
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Radioactivity
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The second mystery of Ettore Majorana
In 1937, Majorana [2] theoretically showed that the conclusions ofthe theory of β decay remain unchanged under the assumption of the existence of only one type of the neutrino having no antiparticle
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e e
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→ → <= =>
Majorana =>1937
Dirac or Majorana neutrino?
RIGHT
LEFT:
:
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EXO-200 => 2.71±0.017(stat.)±0.06(sys.)×1021 yr.
Kamland-Zen 2.38 ± 0.02(stat) ± 0.14(syst) × 1021 yr GERDA I 1.84 +0.14 -10(stat) × 1021 yr
21Benasque March 19,2015 Ettore Fiorini
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Neutrino oscillations
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Sterile neutrinosLSND,Miniboon,Gallex,reactors
Great discovery requires great evidence (P. de Bernardis)
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<m> ~ 0.34eV
Bracking news then 0 in 76Ge
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GERDA
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Complain by H.Klapdor
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Future experiments on DBD
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GERDA Majorana Supernemo
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SNO+
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NEXT
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Incident particle
absorber crystal
Thermal sensor
Energy resolution <1 eV ~ 1eV @ 6 keV ~10 eV ~keV @ 2 MeV
VC
Q T
J/K )( v
v 1944 C 3
m V
T
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Thermal detectors
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CUORICINO CUORE0 CUORE
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Hybrid techniquesHeat+ scintillation , light, Cherenkov light
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Ettore Fiorini 40
Crystal made from
ββ-isotopes
Thermometer
Light detector
Heat sink
Heat sink
0νββ emitters: 130Te, 82Se, 100Mo & few others
Crystals: TeO2 , ZnSe, ZnMoO4, CaMoO4
Operation at <20 mK:
Cuore (w/o light detection)
Lucifer, Lumineu, Amore(with light detection)
Lucifer
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Qββ (82Se) = 2995 keVArray of 32-36 enr. (95%) Zn82Se crystals
Total 82Se nuclei: (6.7-8.0) 1025
Single detector: 460 gBI (goal): 1-2 x10-3 cts / (keV kg yr)
ΔE (FWHM): 10-15 keV • Bgd (internal α’s):17.2±4.6 μBq/kg (232Th)24.6±5.5 μBq/kg (238U)• Isotope delivery:
9/15 kg 82Se delivered final batch for
02/2015 • Crystal growth:
Schedule for Jan - June 2015Current yield: 70%
‘anomalous β/γ-quenching’
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Now a competitor AMORE
Advanced Mo based Rare process Experiment
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Before the nightmareFrancesco Jachello entering the field
The nightmare of matrix elements
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Robertson idea
4444Benasque March 19,2015 Ettore Fiorini
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Ettore Fiorini 46
Is Francesco Iachello right ?
Amicus Plato, sed magis amica veritasPlato is a friend , but truth even a better one
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Detectors of unprecedentent sensitivity Environmental radioactivity Trace elements Archaeometry
Reactors => friends and enemiesIs neutrinoless double beta decay the only way to test lepton conservation?
A possible experiment to search
e =>
A favor to be returned => reactor physics
=> Measurement of the position of the fire inside the reactor=> Displacement of the Uranium column in the core
Majorana neutrino and consequences
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Ettore Fiorini
Radionuclide OriginGamma Peak (keV)
Branching ratios (%)
Absolute detection efficiency εabs (%)
Min (μ Bqm−3)Max (μ Bqm−3)
Mean (μ Bqm−3)
7Be Cosmogenic 477 10.3 0.69 ± 0.10 200 ± 40 970 ± 190 470 ± 90
131I Fukushima284 81.2 1.08 ± 0.16 23 ± 4 410 ± 82 82 ± 16
364 60.6 0.88 ± 0.13
134Cs Fukushima604 97.6 0.57 ± 0.09 1.3 ± 0.3 80 ± 16 9.2 ± 1.8
796 85.4 0.47 ± 0.07
136Cs Fukushima 818 100 0.46 ± 0.07 0.005 ± 0.001
137Cs Fukushima 661 84.6 0.54 ± 0.08 1.6 ± 0.3 93 ± 19 10 ± 2
The Fukushima accident. Agreement by groups =>Measurements of air contamination in Osaka, Berkeley, Seattle etc. Only partially related to the distance Detection of air contamination a factor of million less in Milan with respect to Fukushima
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Majorana theory for electron and positron
Application to neutrino => can a ½ spin particle be its own antiparticle? In superconductors Cooper pairs, being boson like particles, form condensates. Cooper pairs can be added to semiconductors with hole producing spin ½ exitons.Superconductors can contain magnetic wires acting as quasiparticlesCan the Majorana rule be applied to these quasiparticles?
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Massive detectors (now expensive) of unique sophistication
The reduction of the background which could hide neutrinolessevents has reached an unprecedented sensistivity
The quenching due to the new value assummed for gA could reduce the expecttion of the neutrino mass limit by a factor 4 to 5. If true it strongly reduces our hope to reach the invers hierarchy region
The validity to extend to neutrinoles DBD the gA obtained from
two neutrino and single beta decay should be justified
The sophistication reached and to be reached in serches for DBD could have appplications in other fields of science
Aplication to solid state physics of the Maiorana theory could bring to results as important as in elementary particle physics
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Conclusions
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There are more things in Earth and Heaven , Polonius, that can be dreamt of by your Philosophy Hamlet
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