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

Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun (Nature cover)

Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun Nature volume 587, pages 577-582 (2020) published 25 November 2020 [doi:10.1038/s41586-020-2934-0] (full text here) Data availability The datasets generated during the current study are freely available: see

CNO and pep neutrino spectroscopy in Borexino: Measurement of the deep-underground production of cosmogenic 11C in an organic liquid scintillator

CNO and pep neutrino spectroscopy in Borexino: Measurement of the deep-underground production of cosmogenic 11C in an organic liquid scintillator H. Back et al. (Borexino Collaboration) Phys. Rev. C 74, 045805 – Published 11 October 2006 [DOI: 10.1103/PhysRevC.74.045805] (local copy, preprint on arXiv: arXiv:hep-ex/0601035)