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Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II

  • the Borexino collaboration
  • Institute of Physics Bhubaneswar
  • Homi Bhabha National Institute
  • ICTP
  • Cluster of Excellence E-conversion
  • National Research Centre "Kurchatov Institute"
  • Forschungszentrum Jülich (FZJ)
  • University of Milan
  • Department of Chemical Engineering
  • Universität Hamburg
  • Laboratori Nazionali del Gran Sasso
  • Universidad Autónoma de Madrid
  • Princeton University
  • Istituto Nazionale per la Fisica della Materia
  • Virginia Polytechnic Institute and State University
  • Moscow State University
  • University of Hawaii
  • Petersburg Nuclear Phys. Inst.
  • Gran Sasso Science Institute
  • Joint Inst. for Nuclear Research
  • Université Paris Diderot
  • University of Tübingen
  • Johannes Gutenberg University
  • University of Houston
  • Jagiellonian University
  • RWTH Aachen University
  • Forestry Academy of Sciences of Ukraine
  • Wigner Research Centre for Physics
  • National Research Nuclear University MEPhI
  • Fermi National Accelerator Laboratory
  • Technische Universität Dresden
  • INFN Sezione di Perugia
  • University of Massachusetts Amherst
  • Universita La Sapienza
  • Institute of Theoretical Physics Chinese Academy of Sciences
  • Brown University
  • Università degli Studi di Napoli Federico II

Research output: Contribution to journal › Article › peer-review

32 Scopus citations

Abstract

The Borexino detector measures solar neutrino fluxes via neutrino-electron elastic scattering. Observed spectra are determined by the solar-νe survival probability Pee(E), and the chiral couplings of the neutrino and electron. Some theories of physics beyond the Standard Model postulate the existence of Non-Standard Interactions (NSI’s) which modify the chiral couplings and Pee(E). In this paper, we search for such NSI’s, in particular, flavor-diagonal neutral current interactions that modify the νee and ντe couplings using Borexino Phase II data. Standard Solar Model predictions of the solar neutrino fluxes for both high- and low-metallicity assumptions are considered. No indication of new physics is found at the level of sensitivity of the detector and constraints on the parameters of the NSI’s are placed. In addition, with the same dataset the value of sin2θW is obtained with a precision comparable to that achieved in reactor antineutrino experiments [Figure not available: see fulltext.].

Original languageEnglish
Article number38
JournalJournal of High Energy Physics
Volume2020
Issue number2
DOIs
StatePublished - 1 Feb 2020
Externally publishedYes

Keywords

  • Beyond Standard Model
  • Neutrino Physics

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