Identification of the cosmogenic 11C background in large volumes of liquid scintillators with Borexino Eur. Phys. J. C 81, 1075 (2021). [doi: 10.1140/epjc/s10052-021-09799-x] Published 07 December 2021 (preprint on arXiv) Abstract Cosmogenic radio-nuclei are an important source of background for low-energy
Cosmogenic Backgrounds in Borexino at 3800 m water-equivalent depth Journal of Cosmology and Astroparticle Physics, Volume 2013, August 2013 Cit.: G. Bellini et al JCAP08(2013)049 Published 27 August 2013 [doi:10.1088/1475-7516/2013/08/049] (preprint on arXiv) Abstract The solar neutrino experiment Borexino, which is
Production and characterization of a custom-made 228Th source with reduced neutron source strength for the Borexino experiment W. Maneschg, L. Baudis, R. Dressler, K. Eberhardt, R. Eichler, H. Keller, R. Lackner, B. Praast, R. Santorelli, J. Schreiner, M. Tarka, B.
Cosmic-muon flux and annual modulation in Borexino at 3800 m water-equivalent depth G. Bellini et al JCAP05(2012)015 Journal of Cosmology and Astroparticle Physics, Volume 2012, May 2012 doi:10.1088/1475-7516/2012/05/015 (preprint arXiv:1202.6403) Abstract We have measured the muon flux at the underground Gran Sasso National
Muon and cosmogenic neutron detection in Borexino G. Bellini et al 2011 JINST 6 P05005 Journal of Instrumentation, Volume 6, May 2011 Published 11 May 2011 doi:10.1088/1748-0221/6/05/P05005 (preprint on arXiv) Abstract Borexino, a liquid scintillator detector at LNGS, is designed for the detection of neutrinos and
Measurements of extremely low radioactivity levels in BOREXINO. New low-level detection limits for isotopes of interest are obtained.
The design of Borexino, the various facilities essential to its operation, its spectroscopic and background suppression capabilities and a prognosis of the impact of its results towards resolving the solar neutrino problem. Borexino will also address several other frontier questions in particle physics, astrophysics and geophysics.