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

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

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

For most of their existence, stars are powered by fusion of hydrogen into helium via two processes that are well understood theoretically: the proton–proton chain, dominant in relatively small stars like our Sun, and the Carbon–Nitrogen–Oxygen cycle, which is prevalent in bigger, more massive stars. Borexino got the first experimental evidence of neutrinos emitted by the CNO cycle in the Sun core.

Simultaneous precision spectroscopy of pp, 7Be and pep solar neutrinos with Borexino Phase-II

Simultaneous precision spectroscopy of pp, 7Be and pep solar neutrinos with Borexino Phase-II Phys. Rev. D 100, Issue 8 , 082004 – 15 October 2019 [doi:10.1103/PhysRevD.100.082004] Abstract We present the simultaneous measurement of the interaction rates pp, RBe, Rpep of pp, 7Be, and pep solar neutrinos performed with a global fit to the

Comprehensive measurement of pp-chain solar neutrinos

 Comprehensive measurement of pp-chain solar neutrinos Nature volume 562, pages 505–510 (2018) Published: 24 October 2018 [doi:10.1038/s41586-018-0624-y] (full text here) Data availability The datasets generated during the current study are freely available: see below.  Additional information is available from the Borexino Collaboration

Neutrinos from the primary proton-proton fusion process in the Sun

Neutrinos from the primary proton-proton fusion process in the Sun Nature 512, 383-386 (28 August 2014) doi:10.1038/nature13702 Data availability: The datasets generated during the current study are freely available (see below). Additional information is available from the Borexino Collaboration spokesperson (spokesperson-borex@lngs.infn.it)

First evidence of pep solar neutrinos by direct detection in Borexino

First Evidence of pep Solar Neutrinos by Direct Detection in Borexino G. Bellini et al. (Borexino Collaboration) Phys. Rev. Lett. 108, 051302 Published 2 February 2012 doi:10.1103/PhysRevLett.108.051302  (preprint on arXiv) this paper have been been highlighted with a Synopsis on the Physics website:

Measurement of the solar 8B neutrino rate with a liquid scintillator target and 3 MeV energy threshold in the Borexino detector

Measurement of the solar 8B neutrino rate with a liquid scintillator target and 3 MeV energy threshold in the Borexino detector G. Bellini et al. (Borexino Collaboration) Phys. Rev. D 82, 033006 – Published 5 August 2010 doi:10.1103/PhysRevD.82.033006 (local copy;  preprint on arXiv) Abstract