A novel approach in the detection of muon neutrino to tau neutrino oscillation from extragalactic neutrinos

Details A novel approach in the detection of muon neutrino to tau neutrino oscillation from extragalactic neutrinos A novel approach in the detection of muon neutrino to tau neutrino oscillation from extragalactic neutrinos

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phdt.........2i&link_type=abstract

Thesis (PhD). THE UNIVERSITY OF ARIZONA, Source DAI-B 62/06, p. 2773, Dec 2001, 153 pages.

Mathematics

Logic

Scientific paper

A novel approach is proposed for studying the νμ --> ν τ oscillation and detection of extragalactic neutrinos. Active Galactic Nuclei (AGN), Gamma Ray Bursters (GRB) and Topological Defects are believed to be sources of ultrahigh energy νμ and ντ. These astrophysical sources provide a long baseline of 100Mpc, or more, for possible detection of νμ --> ντ oscillation with mixing parameter Δm2 down to 10 -17 eV2, many orders of magnitude below the current accelerator experiments. The propagation characteristics of upward going muon and tau neutrinos is studied to show that high energy tau neutrinos cascade down in energy as they propagate through the Earth, producing an enhancement of the incoming tau neutrino flux in the low energy region. By contrast, high energy muon neutrinos get attenuated as they traverse the Earth. It is observed that the relative steepness of the incoming neutrino flux spectrum and the nadir angle of the Earth are two important factors that influence the enhancement and cascade of ντ flux. This effect provides a novel way to search for tau neutrino appearance by measuring the angular dependence of tau neutrino induced upward muons; and upward hadronic and electromagnetic showers. A Monte Carlo evaluation of tau survival probability and its range shows that at energies below 107-10 8 GeV, depending on the material, only tau decays are important. However, at higher energies the tau energy losses are significant, hence reducing the survival probability of tau. Here, tau energy loss for energies up to 10 9 GeV have been calculated taking into consideration the decay of tau. An understanding of tau energy loss at very high energies could help with the interpretation of long tracks produced by charged particles in large underground detectors.

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