Fabio Mantovani
University of Ferrara
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Featured researches published by Fabio Mantovani.
Physics Letters B | 2013
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
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
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. 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
G. Fiorentini; Fabio Mantovani; B. Ricci
{10}^{32}\mathrm{proton}\mathrm{yr}
Physical Review D | 2012
G. Fiorentini; Fabio Mantovani; G. L. Fogli; E. Lisi; A. M. Rotunno
and 100% efficiency assuming
Physical Review D | 2005
Gianni Fiorentini; M. Lissia; Fabio Mantovani; Riccardo Vannucci
{\mathrm{sin}}^{2}(2\ensuremath{\theta})=0.863
Journal of Radioanalytical and Nuclear Chemistry | 2016
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
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
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.