Ultra-low background gamma spectrometry 2 nd LSM-Extension Workshop, Valfréjus, 16 October 2009 Pia Loaiza Laboratoire Souterrain de Modane.

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Ultra-low background gamma spectrometry 2 nd LSM-Extension Workshop, Valfréjus, 16 October 2009 Pia Loaiza Laboratoire Souterrain de Modane

Pia Loaiza, 2 nd LSM-Extension Workshop,Valfréjus, October 16th,  U,Th,K (n, ,  ) Shielding close mat. e-e- n Det. Sources of radioactive background Rn External gamma radiation, neutrons Rn and its progenies Radioimpurities in shielding materials Radioimpurities in materials close to detectors Contaminants in detector itself Need material screening

Pia Loaiza, 2 nd LSM-Extension Workshop,Valfréjus, October 16th, U decay chain Gamma emitters Mass spectrometry, Neutron Activation Analysis, Alpha-spectrometry Sub-chains

Pia Loaiza, 2 nd LSM-Extension Workshop,Valfréjus, October 16th, Th decay chain Gamma emitters Sub-chains Mass spectrometry, NAA, Alpha spectrometry NA: typical limits,Th: some ppb

Pia Loaiza, 2 nd LSM-Extension Workshop,Valfréjus, October 16th, Ge spectrometry Best limits 226Ra, 228Th : 20  Bq/kg for measurement time 100 days and 125 kg of Cu  Backg. R . I. M.  t R = resolution  = efficiency I = intensity of the line M = sample mass t = time of measurement For all types: To improve sensitivity  BACKGROUND REDUCTION COAXIALWELL PLANAR high sample mass high efficiency high resolution at low energies The choice depends on what we want to measure Detection Limit 

Pia Loaiza, 2 nd LSM-Extension Workshop,Valfréjus, October 16th, Background components in Ge spectrometry deep underground 2.6 MeV DET.  e-e- neutron 210 Bi ( 210 Pb) -- 511 keV Rn e-e- e+e+ Pb External gamma radiation (up to 2.6 MeV 208 Tl) neutrons from fission and ( ,n) reactions Rn and its progenies Radioimpurities in the shielding materials Radioimpurities in cryostat MOST IMPORTANT : MATERIAL SELECTION Done in iterative steps Mass = 140 kg Mass = 1125 kg

Pia Loaiza, 2 nd LSM-Extension Workshop,Valfréjus, October 16th, Which sensitivities for the future experiments? EURECA: Present  rejection factor ~ 10 5 According to simulations: ~10 5 evts/year in 10 keV<E<50 keV in 1000 kg of Ge from Cu 226Ra, 228Th : 20  Bq/kg The necessary sensitivity levels are reached, but time-consuming measurements needed need more detectors SuperNEMO 40 mBq/kg in 214Bi 3 mBq/kg in 228Th needed for PMTS further reduce background?

Pia Loaiza, 2 nd LSM-Extension Workshop,Valfréjus, October 16th, Experiment-specific radioctivity measurements Example: the BiPo detector for SuperNEMO Measurement of 208 Tl and 214 Bi concentration in foil-sources and other thin materials Goal : measurement of 10 m 2 of foil-sources (40 mg/cm2) in 1 month with sensibility : –Volume concentrations : 208Tl < 2  Bq/kg & 214Bi < 10  Bq/kg Detection of the BiPo cascade :  + delayed    Plastic scintillateursSource foil

Pia Loaiza, 2 nd LSM-Extension Workshop,Valfréjus, October 16th, Conclusions Gamma-spectrometry: non destructive technique of measurement of low radioactivities Sensibilities needed for future experiments are reached Need probably a large number of detectors AND detector-specific methods

Pia Loaiza, 2 nd LSM-Extension Workshop,Valfréjus, October 16th, Ni: % IN ORE< !-2 ppm Co:about 5 ppm < 1 ppm 40 K:7.5  1.0 mBq/kg< mBq/kg 226 Ra:1.8  0.4 mBq/kg< mBq/kg 228 Th:< 0.44 mBq/kg< mBq/kg Copper: FROM G. HEUSSER % ppm O NOSV quality % (1-4 ppm O 2 ) Aluminium PHP: 40 K – 0.1 mBq/kg 226 Ra 0.27  0.19 mBq/kg 228 Ra < 0.11 mBq/kg 228 Th 1.4  0.2 mBq/kg Stainless steel: (From G. Heusser): 40 K 17+/-3 mBq/kg1.8+/-6 mBq/kg 226 Ra < 1 mBq/kg0.6+/-0.2 mBq/kg 228 Ra 228 Th < 1 mBg/kg0.2+/-0.1 mBq/kg 60 Co 12+/-5 mBq/kg18+/-1 mBq/kg