"Geo-neutrinos, electron anti-neutrinos produced in β decays of naturally occurring radioactive isotopes in the Earth, are a unique direct probe of our planet’s interior. We report the first observation at morethan 3σ C.L. of geo-neutrinos, performed with the Borexino detector at Laboratori Nazionali del GranSasso. Anti-neutrinos are detected through the neutron inverse β decay reaction. With a 252.6 ton yr fiducial exposure after all selection cuts, we detected 9.9+4.1 (+14.6 ) geo-neutrino events, with errors −3.4 −8.2 corresponding to a 68.3% (99.73%) C.L. From the ln L profile, the statistical significance of the Borexino geo-neutrino observation corresponds to a 99.997% C.L. Our measurement of the geo-neutrinos rate is 3.9+1.6 (+5.8 ) events/(100 ton yr). The observed prompt positron spectrum above 2.6 MeV is compatible with that expected from European nuclear reactors. Our measurement of reactor anti-neutrinos excludes the non-oscillation hypothesis at 99.60% C.L. This measurement rejects the hypothesis of an active geo-reactor in the Earth’s core with a power above 3 TW at 95% C.L."

Observation of geo neutrinos

FIORENTINI, Giovanni;RICCI, Barbara;
2010

Abstract

"Geo-neutrinos, electron anti-neutrinos produced in β decays of naturally occurring radioactive isotopes in the Earth, are a unique direct probe of our planet’s interior. We report the first observation at morethan 3σ C.L. of geo-neutrinos, performed with the Borexino detector at Laboratori Nazionali del GranSasso. Anti-neutrinos are detected through the neutron inverse β decay reaction. With a 252.6 ton yr fiducial exposure after all selection cuts, we detected 9.9+4.1 (+14.6 ) geo-neutrino events, with errors −3.4 −8.2 corresponding to a 68.3% (99.73%) C.L. From the ln L profile, the statistical significance of the Borexino geo-neutrino observation corresponds to a 99.997% C.L. Our measurement of the geo-neutrinos rate is 3.9+1.6 (+5.8 ) events/(100 ton yr). The observed prompt positron spectrum above 2.6 MeV is compatible with that expected from European nuclear reactors. Our measurement of reactor anti-neutrinos excludes the non-oscillation hypothesis at 99.60% C.L. This measurement rejects the hypothesis of an active geo-reactor in the Earth’s core with a power above 3 TW at 95% C.L."
2010
G., Bellini; J., Benzigerm; S., Bonetti; M., Buizza Avanzini; B., Caccianigah; L., Cadonati; F. Calapricel C., Carraroc; A., Chavarrial; F., Dalnoki Veressl; 1, ; D., D'Angeloh; S., Davini; H., de Kerreta; A., Derbink; A., Etenkof; Fiorentini, Giovanni; K., Fomenkob; D., Francoh; C., Galbiati; S., Gazzanag; C., Ghianog; M., Giammarchi; M., Goeger Nei; A., Goretti; E., Guardincerri; S., Hardyo; Aldo, Ianni; Andrea, Ianni; M., Joyceo; V. V., Kobychevr; Y., Koshioq; G., Korgag; D., Kryna; M., Leungl; T., Lewkei; E., Litvinovichf; B., Loerl; P., Lombardi; L., Ludhovah; I., Machulinf; S., Manecki; W., Maneschgd; G., Manuzioc; Q., Meindl; E., Meroni h; L., Miramonti h; M., Misiaszeke; D., Montanari; V., Muratovak; L., Oberaueri; M., Obolenskya; F., Orticaj; M., Pallavicini; L., Pappg; L., Perassoh; S., Perassoc; A., Pocarn; R. S., Raghavano; G., Ranucci; A., Razetog; A., Reh; Ricci, Barbara; P., Rissoc; A. Romani, J.; D., Rountreeo; A., Sabelnikovf; R., Saldanhal; C., Salvoc; S., Schonertd; H., Simgend; M., Skorokhvatovf; O., Smirnovb; A., Sotnikovb; S., Sukhotinf; Y., Suvorovh; R., Tartagliag; G., Testerac; D., Vignauda; R. B., Vogelaaro; F., von Feilitzschi; J., Winteri; M., Wojcike; A., Wrightl; M., Wurmi; J., Xul; O., Zaimidorogab; S., Zavatarelli; G., Zuzel
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11392/1388655
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