Spectroscopy of geo-neutrinos from 2056 days of Borexino data
Borexino collaboration, M. Agostini, S. Appel, G. Bellini, J., Benziger, D. Bick, G. Bonfini, D. Bravo, B. Caccianiga, F. Calaprice, A., Caminata, P. Cavalcante, A. Chepurnov, K. Choi, D. DAngelo, S. Davini, A., Derbin, L. Di Noto, I. Drachnev, A. Empl, A. Etenko, G. Fiorentini

TL;DR
This paper reports an improved measurement of geo-neutrinos using 2056 days of Borexino data, providing insights into Earth's radiogenic heat and mantle composition with high statistical significance.
Contribution
The study presents the most precise geo-neutrino measurement from Borexino to date, including a significant detection of mantle geo-neutrinos and constraints on Earth's radiogenic heat production.
Findings
Detection of 23.7 geo-neutrino events with high significance
Evidence for mantle geo-neutrino signal at 98",
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Abstract
We report an improved geo-neutrino measurement with Borexino from 2056 days of data taking. The present exposure is protonyr. Assuming a chondritic Th/U mass ratio of 3.9, we obtain geo-neutrino events. The null observation of geo-neutrinos with Borexino alone has a probability of (5.9). A geo-neutrino signal from the mantle is obtained at 98\% C.L. The radiogenic heat production for U and Th from the present best-fit result is restricted to the range 23-36 TW, taking into account the uncertainty on the distribution of heat producing elements inside the Earth.
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