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Measuring Flavor Ratios of High-Energy Astrophysical Neutrinos
- J. Beacom, N. Bell, D. Hooper, S. Pakvasa, T. Weiler
- Physics
- 1 July 2003
We discuss the prospects for next generation neutrino telescopes, such as IceCube, to measure the flavor ratios of high-energy astrophysical neutrinos. The expected flavor ratios at the sources are…
An evaluation of the exposure in nadir observation of the JEM-EUSO mission
- J. Adams, S. Ahmad, A. Z. Marchi
- Physics
- 1 April 2013
Cosmic neutrino pevatrons: A brand new pathway to astronomy, astrophysics, and particle physics
- L. Anchordoqui, V. Barger, T. Weiler
- Physics
- 23 December 2013
Resonant absorption of cosmic-ray neutrinos by the relic-neutrino background
- T. Weiler
- Physics
- 19 July 1982
Within the framework of standard big-bang cosmology and the standard electroweak model, it is shown that ..nu..nu-bar annihilation on the Z resonance is the only cosmic-ray process sensitive to relic…
Neutrinos as a diagnostic of high energy astrophysical processes [rapid communication]
- L. Anchordoqui, H. Goldberg, F. Halzen, T. Weiler
- Physics
- 1 October 2004
Probing Planck scale physics with IceCube
- L. Anchordoqui, H. Goldberg, T. Weiler
- Physics
- 17 June 2005
Neutrino oscillations can be affected by decoherence induced e.g. by Planck scale suppressed interactions with the space-time foam predicted in some approaches to quantum gravity. We study the…
TeV γ rays and neutrinos from photodisintegration of nuclei in Cygnus OB2
- L. Anchordoqui, J. Beacom, H. Goldberg, S. Palomares-Ruiz, T. Weiler
- Physics
- 20 November 2006
TeV {gamma}-rays may provide significant information about high energy astrophysical accelerators. Such {gamma}-rays can result from the photo-de-excitation of PeV nuclei after their parents have…
Pinning down the cosmic ray source mechanism with new IceCube data
- L. Anchordoqui, H. Goldberg, Morgan H. Lynch, A. Olinto, T. Paul, T. Weiler
- Physics
- 20 June 2013
Very recently the IceCube Collaboration has reported an observation of 28 neutrino candidates with energies between 50 TeV and 2 PeV, constituting a 4.1$\sigma$ excess compared to the atmospheric…
Decay of high-energy astrophysical neutrinos.
- J. Beacom, N. Bell, D. Hooper, S. Pakvasa, T. Weiler
- PhysicsPhysical review letters
- 19 November 2002
TLDR
Measuring flavor ratios of high-energy astrophysical neutrinos
- J. Beacom, N. Bell, D. Hooper, S. Pakvasa, T. Weiler
- Physics
- 11 November 2003
We discuss the prospects for next generation neutrino telescopes, such as IceCube, to measure the flavor ratios of high-energy astrophysical neutrinos. The expected flavor ratios at the sources are…
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