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Searching for long wavelength neutrino oscillations in the distorted neutrino spectrum of galactic supernova remnants

Jun, 2001
38 pages
Published in:
  • Astrophys.J.Suppl. 141 (2002) 147-155
e-Print:
DOI:
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Abstract: (arXiv)
We investigate the muon neutrino event rate in km3^3 neutrino telescopes due to a number of galactic supernova remnants expected on the basis of these objects' known γ\gamma-ray signals. We evaluate the potential of these neutrino signals to exhibit evidence of the sub-dominant neutrino oscillations expected in various neutrino mixing schemes including pseudo-Dirac scenarios and the Exact Parity Model. With ten years' data, neutrino signals from Sgr A East should either discover or exclude neutrino oscillations governed by a δm2\delta m^2 parameter in the range 10−1210^{-12} to 10−1510^{-15} eV2^2. Such a capability is not available to terrestrial or solar system neutrino experiments.
  • supernova
  • galaxy
  • neutrino: cosmic radiation
  • neutrino: particle source
  • neutrino: oscillation
  • neutrino: atmosphere
  • neutrino: solar
  • neutrino: flux
  • neutrino: mass difference
  • counters and detectors: resolution
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