IS THE NEUTRINO A MAJORANA OR A DIRAC PARTICLE ? Ettore Fiorini, Bologna June 17 2005 or Lepton number conservation or violation Has neutrino a finite.

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Presentation transcript:

IS THE NEUTRINO A MAJORANA OR A DIRAC PARTICLE ? Ettore Fiorini, Bologna June or Lepton number conservation or violation Has neutrino a finite mass 100 % chirality

The Standard Model e ֿ e ֿ ֿ Flavor conservation or violation Neutrino oscillations need m 0 e

Neutrino oscillations have been observed with solar, atmosperic and reactor neutrinos

ATMOSPHERIC NEUTRINOS Superkamiokande and MACRO Reactor and long baseline experiments Neutrino factories

1. (A,Z) => (A,Z+2) + 2 e e ¯ 2. (A,Z) => (A,Z+2) + 2 e - + ( …2,3 3. (A,Z) => (A,Z+2) + 2 e - But oscillation experiments only indicate that m 2 0 to determine => double beta decay

0 - decay e - e - d d u u W W e e Neutrinoless decay

Neutrinoless decay would imply a non zero effective majorana neutrino mass as indicated by oscillation experiments

Experimental approaches Direct experiments Source detector Source = detector (calorimetric) Geochemical experiments i82 Se = > 82 Kr, 96 Zr = > 96 Mo (?), 128 Te = > 128 Xe (non confirmed), 130 Te = > 130 Te Radiochemical experiments 238 U = > 238 Pu (non confirmed) e-e- e-e- e-e- e-e- source detector Source Detector

Incident particle absorber crystal heat bath Thermal sensor Cryogenic detectors

@ 5 keV ~100 mk ~ 1 mg <1 eV ~ 5 2 MeV ~10 mk ~ 1 kg <10 eV ~ keV

m* ee (eV) < 6.0 > Ca Osawa I. et al Experim < 1.0 Belli et al < 0.8 – 2.4 > Xe Range m ee 1/2 0 (y) Isotope < 1.5 Mi DBD – 2002 < 0.9 – 2.1 > Te < 1.0 Bernatowicz et al (GEO) < 1.0 – 4.4 > Te geo < 1.7 Bizzeti et al < 1.6 – 5.5 > Cd < 4.8 Ejiri et al < > Mo < 0.38 IGEX 2002 < 0.3 – 2.5 > < 0.35 Heidelberg – Moscow 2001 < 0.3 – 2.5 > Ge * Staudt, Muto, Klapdor-Kleingrothaus Europh. Lett 13 (1990) 31 Recent experiments on The Klapdor effect => = 1.2 x 1025 a => ~ 0.44 eV

Two new experiments NEMO III e CUORICINO

Searches with thermal detectors Cuoricino (Hall A) CUORE (Hall A) CUORE R&D (Hall C)

Crescita della massa dei bolometri year total mass [kg]

11 modules, 4 detector each, crystal dimension 5x5x5 cm 3 crystal mass 790 g 4 x 11 x 0.79 = kg of TeO 2 2 modules, 9 detector each, crystal dimension 3x3x6 cm 3 crystal mass 330 g 9 x 2 x 0.33 = 5.94 kg of TeO 2 Search for the 2 | o in 130 Te (Q=2529 keV) and other rare events At Hall A in the Laboratori Nazionali del Gran Sasso (LNGS) 18 crystals 3x3x6 cm crystals 5x5x5 cm3 = 40.7 kg of TeO2 Operation started in the beginning of 2003 => ~ 4 months Background.18±.01 c /kev/ kg/ a T 1/2 0 ( 130 Te) > 1.8x y Klapdor 0.1 – 0.9

Cosmological disfavoured region (WMAP) Direct hierarchy m 2 12 = m 2 sol Inverse hierarchy m 2 12 = m 2 atm quasi degeneracy m 1 m 2 m 3 With the same matrix elements the Cuoricino limit is 0.53 eV Present Cuoricino region Possible evidence (best value 0.39 eV) Feruglio F., Strumia A., Vissani F. hep-ph/ Arnaboldi et al., submitted to PRL, hep-ex/ (2005).

The CUORE project 988 bolometers in 19 colums od 13 flors of 4 crystals 750 kg TeO 2 => 600 kg Te => 203 kg 130 Te Sensitivity of a few tens of eV

The discovery of neutrino oscillations to which Masatoshi contributed so much exists and m 2 0 We need to determine the Majorana nature of the neutrino and the absolute value of Neutrinoless double beta decay would indicate not only lepton number violation, but also m 0 This process has been indicated by an experiment (Klapdor) with a value of ~0.44 eV but not confirmed by CUORICINO Future experiments on neutrinoless double beta decay will allow to reach the sensitivity predicted by oscillations Their peculiar multiplinarity involves nuclear and e subnuclear physics, astrophysics, radioactivity, material science, geochronology etc CONCLUSIONS