Distributions for tau neutrino interactions observed through the decay τ→μντν¯μ

  title={Distributions for tau neutrino interactions observed through the decay $\tau$→$\mu$$\nu$$\tau$$\nu$¯$\mu$},
  author={I. Alikhanov and Emmanuel Anthony Paschos},
  journal={Physics Letters B},
3 Citations

Impact of nuclear gluon distributions on leptoquark production by neutrinos

We investigate non-standard interactions of neutrinos with atomic nuclei through excitations of leptoquarks. A leptoquark term in the Lagrangian admits the possibility that neutrinos interact with

Lepton Pair Production in Neutrino–Nucleus Scattering

Open Issues in Neutrino Reactions

Numerous investigations discuss neutrino properties from low to ultra high energies. This review discusses several topics that are investigated in present day experiments. The first section covers



Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector

The presence of a high-energy neutrino flux containing the most energetic neutrinos ever observed is revealed, including 28 events at energies between 30 and 1200 TeV, although the origin of this flux is unknown and the findings are consistent with expectations for a neutRino population with origins outside the solar system.

Standard model explanation of the ultrahigh energy neutrino events at IceCube

The recent observation of two PeV events at IceCube, followed by an additional 26 events between 30 - 300 TeV, has generated considerable speculations on its origin, and many exotic New Physics


Evidence for an extraterrestrial flux of high-energy neutrinos has now been found in multiple searches with the IceCube detector. The first solid evidence was provided by a search for neutrino events

Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube.

A shower-biased sample containing 129 showers and 8 tracks collected in three years from 2010 to 2013 is obtained and consistency with the (fe:fμ:fτ):fτ flavor ratio at Earth commonly expected from the averaged oscillations of neutrinos produced by pion decay in distant astrophysical sources is demonstrated.

Erratum: Measuring flavor ratios of high-energy astrophysical neutrinos [Phys. Rev. D 68, 093005 (2003)]

Because of a programming error, some of the results presented in our published paper [1] are incorrect. Here we revise Figs. 1–4,7,8 and some of the associated discussion, including the final column

Observation of high-energy astrophysical neutrinos in three years of IceCube data.

Results from an analysis with a third year of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV-PeV range at the level of 10(-8)  GeV cm-2 s-1 sr-1 per flavor and reject a purely atmospheric explanation for the combined three-year data at 5.7σ.

Atmospheric and Astrophysical Neutrinos above 1 TeV Interacting in IceCube

The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV-PeV) neutLrinos produced in distant astrophysical objects. A search for. greater than or similar to 100 TeV

Decay of high-energy astrophysical neutrinos.

This work states that for lifetimes even several orders of magnitude longer, high-energy neutrinos from distant astrophysical sources would decay, which would strongly alter the flavor ratios from the phi(nu(e)):phi-nu(mu):phi(tau)=1-1:1 expected from oscillations alone and should be readily visible in the near future.

Review of Particle Physics

  • K. Olive
  • Physics, Environmental Science
    Physical review. D, Particles and fields
  • 1996
The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 3,283 new measurements from 899 papers, we list, evaluate, and average measured properties of

Observation of ultrahigh-energy cosmic rays with the ANITA balloon-borne radio interferometer.

Measurements in the 300-900 MHz range are presented, which are the first self-triggered, first ultrawide band, first far-field, and the highest energy sample of cosmic ray events collected with the radio technique.