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Constraining the NuMI neutrino flux using inverse muon decay reactions in MINERvA

  • (The MINERνA Collaboration)
  • University of Rochester
  • College of William and Mary
  • Aligarh Muslim University
  • Pontifical Catholic Univ. of Peru
  • Oregon State University
  • Fermi National Accelerator Laboratory
  • Universidad de Guanajuato
  • University of Geneva
  • Centro Brasileiro de Pesquisas Físicas
  • Brookhaven National Laboratory
  • University of Notre Dame
  • Los Alamos National Laboratory
  • Tufts University
  • Universidad Técnica Federico Santa Maria
  • University of Minnesota Duluth
  • York University Toronto
  • Indian Institute of Science Education and Research Mohali
  • University of Pennsylvania School of Arts and Sciences
  • Rutgers - The State University of New Jersey, New Brunswick
  • University of Oxford
  • Massachusetts College of Liberal Arts
  • University of Pittsburgh
  • University of Minnesota Twin Cities
  • University of Florida
  • Universidad Nacional de Ingenieriá
  • Imperial College of Science Technology and Medicine

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

10 Citas (Scopus)

Resumen

Inverse muon decay, νμe-→μ-νe, is a reaction whose cross section can be predicted with very small uncertainties. It has a neutrino energy threshold of ≈11 GeV and can be used to constrain the high-energy part of the flux in the NuMI neutrino beam. This reaction is the dominant source of events which only contain high-energy muons nearly parallel to the direction of the neutrino beam. We have isolated a sample of hundreds of such events in neutrino and antineutrino enhanced beams, and have constrained the predicted high-energy flux.

Idioma originalInglés
Número de artículo092010
PublicaciónPhysical Review D
Volumen104
N.º9
DOI
EstadoPublicada - 1 nov. 2021

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