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Dive into the research topics where Fabio Mantovani is active.

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Featured researches published by Fabio Mantovani.


Physics Letters B | 2013

Measurement of geo-neutrinos from 1353 days of Borexino

G. Bellini; J. Benziger; D. Bick; G. Bonfini; D. Bravo; M. Buizza Avanzini; B. Caccianiga; L. Cadonati; F. Calaprice; P. Cavalcante; A. Chavarria; A. Chepurnov; D. D'Angelo; S. Davini; A. Derbin; A. Empl; A. Etenko; G. Fiorentini; K. Fomenko; D. Franco; C. Galbiati; S. Gazzana; C. Ghiano; M. Giammarchi; M. Goeger-Neff; A. Goretti; L. Grandi; C. Hagner; E. Hungerford; Aldo Ianni

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 ) × 10 31 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 S geo = ( 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 S Th = ( 10.6 ± 12.7 ) TNU and S U = ( 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 31.2 − 6.1 + 7.0 reactor anti-neutrino events is in agreement with expectations in the presence of neutrino oscillations.


Physical Review D | 2004

Antineutrinos from Earth: A reference model and its uncertainties

Fabio Mantovani; Luigi Carmignani; Gianni Fiorentini; M. Lissia

We predict geoneutrino fluxes in a reference model based on a detailed description of Earths crust and mantle and using the best available information on the abundances of uranium, thorium, and potassium inside Earths layers. We estimate the uncertainties of fluxes corresponding to the uncertainties of the element abundances. In addition to distance integrated fluxes, we also provide the differential fluxes as a function of distance from several sites of experimental interest. Event yields at several locations are estimated and their dependence on the neutrino oscillation parameters is discussed. At Kamioka we predict


Physics Reports | 2007

Geo-neutrinos and earth's interior

Gianni Fiorentini; M. Lissia; Fabio Mantovani

N(\mathrm{U}+\mathrm{Th})=35\ifmmode\pm\else\textpm\fi{}6


Science of The Total Environment | 2012

A new FSA approach for in situ γ ray spectroscopy.

A. Caciolli; Marica Baldoncini; G. P. Bezzon; C. Broggini; G. P. Buso; Ivan Callegari; Tommaso Colonna; G. Fiorentini; Enrico Guastaldi; Fabio Mantovani; Giovanni Massa; R. Menegazzo; L. Mou; C. Rossi Alvarez; M. Shyti; A. Zanon; Gerti Xhixha

events for


Physics Letters B | 2003

Neutrinos and Energetics of the Earth

G. Fiorentini; Fabio Mantovani; B. Ricci

{10}^{32}\mathrm{proton}\mathrm{yr}


Physical Review D | 2012

Mantle geoneutrinos in KamLAND and Borexino

G. Fiorentini; Fabio Mantovani; G. L. Fogli; E. Lisi; A. M. Rotunno

and 100% efficiency assuming


Physical Review D | 2005

How much uranium is in the Earth? Predictions for geoneutrinos at KamLAND

Gianni Fiorentini; M. Lissia; Fabio Mantovani; Riccardo Vannucci

{\mathrm{sin}}^{2}(2\ensuremath{\theta})=0.863


Journal of Radioanalytical and Nuclear Chemistry | 2016

Calibration of HPGe detectors using certified reference materials of natural origin

Gerti Xhixha; Matteo Alberi; Marica Baldoncini; Kozeta Bode; Elida Bylyku; Florinda Cfarku; Ivan Callegari; Fadil Hasani; S. Landsberger; Fabio Mantovani; Eva Rodriguez; Ferat Shala; Virginia Strati; Merita Xhixha Kaçeli

and


arXiv: High Energy Physics - Phenomenology | 2005

Geo-Neutrinos: a short review

Gianni Fiorentini; M. Lissia; Fabio Mantovani; Riccardo Vannucci

\ensuremath{\delta}{m}^{2}=7.3\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}5}{\mathrm{eV}}^{2}.


Remote Sensing of Environment | 2013

A multivariate spatial interpolation of airborne γ-ray data using the geological constraints

Enrico Guastaldi; Marica Baldoncini; Giampietro Bezzon; C. Broggini; Giampaolo Buso; A. Caciolli; Luigi Carmignani; Ivan Callegari; Tommaso Colonna; Kujtim Dule; G. Fiorentini; Merita Kaçeli Xhixha; Fabio Mantovani; Giovanni Massa; R. Menegazzo; L. Mou; Carlos Rossi Alvarez; Virginia Strati; Gerti Xhixha; A. Zanon

The maximal prediction is 55 events, obtained in a model with fully radiogenic production of the terrestrial heat flow.

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G. Fiorentini

Istituto Nazionale di Fisica Nucleare

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Gerti Xhixha

Istituto Nazionale di Fisica Nucleare

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L. Mou

Istituto Nazionale di Fisica Nucleare

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M. Lissia

Istituto Nazionale di Fisica Nucleare

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B. Ricci

University of Ferrara

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G. P. Bezzon

Istituto Nazionale di Fisica Nucleare

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