We present a measurement of the geo--neutrino signal obtained from 1353 days of data with the Borexino detector at Laboratori Nazionali del Gran Sasso in Italy. With a fiducial exposure of (3.69 ± 0.16) × 1031 proton × year after all selection cuts and background subtraction, we detected (14.3 ± 4.4) geo-neutrino events assuming a fixed chondritic mass Th/U ratio of 3.9. This corresponds to a geo-neutrino signal Sgeo = (38.8 ± 12.0) TNU with just a 6 × 10−6 probability for a null geo-neutrino measurement. With U and Th left as free parameters in the fit, the relative signals are STh = (10.6 ± 12.7) TNU and SU = (26.5 ± 19.5) TNU. Borexino data alone are compatible with a mantle geo--neutrino signal of (15.4 ± 12.3) TNU, while a combined analysis with the KamLAND data allows to extract a mantle signal of (14.1 ± 8.1) TNU. Our measurement of a reactor anti--neutrino signal Sreact = 84.5+19.3−18.9 TNU is in agreement with expectations in the presence of neutrino oscillations.

Measurement of geo-neutrinos from 1353 days of Borexino

FIORENTINI, Giovanni;MANTOVANI, Fabio;RICCI, Barbara;
2013

Abstract

We present a measurement of the geo--neutrino signal obtained from 1353 days of data with the Borexino detector at Laboratori Nazionali del Gran Sasso in Italy. With a fiducial exposure of (3.69 ± 0.16) × 1031 proton × year after all selection cuts and background subtraction, we detected (14.3 ± 4.4) geo-neutrino events assuming a fixed chondritic mass Th/U ratio of 3.9. This corresponds to a geo-neutrino signal Sgeo = (38.8 ± 12.0) TNU with just a 6 × 10−6 probability for a null geo-neutrino measurement. With U and Th left as free parameters in the fit, the relative signals are STh = (10.6 ± 12.7) TNU and SU = (26.5 ± 19.5) TNU. Borexino data alone are compatible with a mantle geo--neutrino signal of (15.4 ± 12.3) TNU, while a combined analysis with the KamLAND data allows to extract a mantle signal of (14.1 ± 8.1) TNU. Our measurement of a reactor anti--neutrino signal Sreact = 84.5+19.3−18.9 TNU is in agreement with expectations in the presence of neutrino oscillations.
2013
G., Bellinia; J., Benzigerb; D., Bickc; G., Bonnid; D., Bravoe; M., Buizza Avanzinif; B., Caccianigaa; L., Cadonatig; F., Calapriceh; P., Cavalcanted;...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11392/1786699
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