Sensitivity to θ13 and δ in the decaying astrophysical neutrino scenario

John F. Beacom, Nicole F. Bell, Dan Hooper, Sandip Pakvasa, and Thomas J. Weiler
Phys. Rev. D 69, 017303 – Published 30 January 2004
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Abstract

We have previously shown that the decay of high-energy neutrinos from distant astrophysical sources would be revealed by flavor ratios that deviate strongly from the φνe:φνμ:φντ=1:1:1 expected from oscillations alone. Here we show that the deviations are significantly larger when the mixing angle θ13 and the CP phase δ are allowed to be nonzero. If neutrinos decay, this could allow measurement of θ13 and δ in IceCube and other near-term neutrino telescopes.

  • Received 23 September 2003

DOI:https://doi.org/10.1103/PhysRevD.69.017303

©2004 American Physical Society

Authors & Affiliations

John F. Beacom1, Nicole F. Bell1, Dan Hooper2, Sandip Pakvasa3, and Thomas J. Weiler4

  • 1NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500, USA
  • 2Denys Wilkinson Laboratory, Astrophysics Department, OX1 3RH Oxford, England
  • 3Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
  • 4Department of Physics and Astronomy, Vanderbilt University, Nashville, Tennessee 37235, USA

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Vol. 69, Iss. 1 — 1 January 2004

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