Borexino’s search for low-energy neutrinos associated with gravitational wave events from GWTC-3 database (Eur. Phys. J. C 83, 538 – 2023). Search for neutrino events in correlation with gravitational wave (GW) events for three observing runs (O1, O2 and O3) from 09/2015 to 03/2020.
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).
Search for low-energy signals from fast radio bursts with the Borexino detector Eur. Phys. J. C 82, 278 (2022). [doi: 10.1140/epjc/s10052-022-10197-0] Published 31 March 2022 Abstract The search for neutrino events in correlation with 42 most intense fast radio
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
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
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.
Search for low-energy neutrinos from astrophysical sources with Borexino Astroparticle Physics Volume 125, February 2021, 102509 [DOI: doi.org/10.1016/j.astropartphys.2020.102509] (Submitted 1 October 2019, Accepted 29 August 2020, Available online 1 September 2020) Abstract We report on searches for neutrinos and antineutrinos
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]
Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II The Borexino CollaborationJournal of High Energy Physics 2020, 38 – Published 5 February 2020 [doi:10.1007/JHEP02(2020)038] (preprint on arXiv) Data availability The datasets generated during the current study are freely available: see below
Comprehensive geoneutrino analysis with Borexino Phys. Rev. D 101, 012009 – Published 21 January 2020 [doi:10.1103/PhysRevD.101.012009] (preprint on arXiv). This paper have been been highlighted with a synopsis: “Earth As a Neutrino Source”. Data availability The datasets generated during the
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
Modulations of the cosmic muon signal in ten years of Borexino data JCAP Volume 2019, February 22, 2019 [doi:10.1088/1475-7516/2019/02/046] (Open Access)
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
A Search for Low-energy Neutrinos Correlated with Gravitational Wave Events GW 150914, GW 151226, and GW 170104 with the Borexino Detector The Astrophysical Journal (ApJ), 850-21, Nov. 2017 Published November 14, 2017 [doi:10.3847/1538-4357/aa9521] (local copy; preprint on arXiv) Abstract We present
The Monte Carlo simulation of the Borexino detector Astroparticle Physics, Volume 97, 2018, Pages 136-159, ISSN 0927-6505 Published 17 October 2017. [doi:10.1016/j.astropartphys.2017.10.003] (preprint on arXiv)
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