Improved Measurement of CNO Solar Neutrinos and Its Implications for the SSM

Improved Measurement of Solar Neutrinos from the Carbon-Nitrogen-Oxygen Cycle by Borexino and Its Implications for the Standard Solar Model Phys. Rev. Lett. 129, 252701 (2022) – Published 12 December 2022 [DOI:10.1103/PhysRevLett.129.252701] This paper have been been highlighted. See Viewpoint: “Elemental

Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino

Independent determination of the Earth’s orbital parameters with solar neutrinos in Borexino Astroparticle Physics Volume 145, March 2023, 102778 ISSN 0927-6505 [doi: 10.1016/j.astropartphys.2022.102778]   Data availability The datasets generated during the current study are freely available: see below (scroll down). Additional

Correlated and integrated directionality for sub-MeV solar neutrinos in Borexino

Correlated and integrated directionality for sub-MeV solar neutrinos in Borexino Phys. Rev. D 105, 052002 – Published 3 March 2022 [doi: 10.1103/PhysRevD.105.052002]   This paper have been been highlighted with a synopsis: “Solar-Neutrino Detection Gets a Boost” Abstract Liquid scintillator detectors play

Identification of the cosmogenic 11C background in large volumes of liquid scintillators with Borexino

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