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 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).
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 a
First Directional Measurement of Sub-MeV Solar Neutrinos with Borexino Phys. Rev. Lett. 128, 091803 – Published 3 March 2022 [doi:10.1103/PhysRevLett.128.091803] This paper have been been highlighted with a synopsis: “Solar-Neutrino Detection Gets a Boost” Abstract We report the measurement of sub-MeV
Sensitivity to neutrinos from the solar CNO cycle in Borexino Eur. Phys. J. C 80, 1091 (2020) [doi:10.1140/epjc/s10052-020-08534-2] published 26 November 2020 (cover story) This paper have been been highlighted on EPJ C Highlight, Springer Research News and Europhysics News
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.
Improved measurement of 8B solar neutrinos with 1.5 kt⋅y of Borexino exposure M. Agostini et al. (Borexino Collaboration) Phys. Rev. D 101, 062001 – Published 6 March 2020 [doi:10.1103/PhysRevD.101.062001]
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 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 (scroll down). Additional information is available from the
Limiting neutrino magnetic moments with Borexino Phase-II solar neutrino data M. Agostini et al. (The Borexino collaboration) Phys. Rev. D 96, 091103(R) – Published 29 November 2017 [doi:10.1103/PhysRevD.96.091103] (preprint on arXiv) Abstract A search for the solar neutrino effective magnetic moment has been
Seasonal modulation of the 7Be solar neutrino rate in Borexino Astroparticle Physics, Volume 92, June 2017, Pages 21-29, ISSN 0927-6505 Published 26 April 2017 [doi:10.1016/j.astropartphys.2017.04.004] (preprint on arXiv) Data availability The datasets generated during the current study are freely available: see
Neutrinos from the primary proton-proton fusion process in the Sun Nature 512, 383-386 (28 August 2014) [doi:10.1038/nature13702] It looks like our results on p-p neutrino measurement have attracted some general public interest. See below for a (likely incomplete) list of articles appeared
Final results of Borexino phase-I on low-energy solar neutrino spectroscopy Phys. Rev. D 89:11 (2014 Jun 25), pp. 112007.1-112007.68 [doi:10.1103/PhysRevD.89.112007] (preprint on arXiv) Abstract Borexino has been running since May 2007 at the Laboratori Nazionali del Gran Sasso laboratory in
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
Absence of a day–night asymmetry in the 7Be solar neutrino rate in Borexino Physics Letters B, Volume 707, Issue 1, 16 January 2012, Pages 22-26 (Submitted 18 October 2011, Revised 10 November 2011, Accepted 13 November 2011, Available online 25 November 2011).
Precision Measurement of the 7Be Solar Neutrino Interaction Rate in Borexino G. Bellini et al. (Borexino Collaboration) Phys. Rev. Lett. 107, 141302 – Published 30 September 2011 [doi:10.1103/PhysRevLett.107.141302] (preprint on arXiv)
Study of solar and other unknown anti-neutrino fluxes with Borexino at LNGS Physics Letters B Volume 696, Issue 3, 31 January 2011, Pages 191-196 [doi:10.1016/j.physletb.2010.12.030] (local copy, preprint on arXiv)
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)
Direct Measurement of the 7Be Solar Neutrino Flux with 192 Days of Borexino Data C. Arpesella et al. (Borexino Collaboration) Phys. Rev. Lett. 101, 091302 – Published 29 August 2008 [doi:10.1103/PhysRevLett.101.091302] (local copy; preprint on arXiv)
First real time detection of 7Be solar neutrinos by Borexino Physics Letters B Volume 658, Issue 4, 3 January 2008, Pages 101-108 (Submitted 10 August 2007, Revised 12 September 2007, Accepted 20 September 2007, Available online 5 October 2007). [doi:10.1016/j.physletb.2007.09.054] (local copy; preprint on