Effect of Resonant Neutrino Oscillation on TeV Neutrino Flavor Ratio from Choked GRBs
arXiv:1007.4582 · doi:10.1088/1674-4527/10/10/001
Abstract
In the collapsar scenario of the long duration Gamma-Ray Bursts (GRBs), multi-TeV neutrino emission is predicted as the jet makes its way through the stellar envelope. Such a neutrino signal is also expected for more general ``failed'' GRBs in which a putative jet is ``choked'' by a heavy envelope. If the ν_e \rightarrow ν_μneutrino oscillation parameters are in the atmospheric neutrino oscillation range, we show that the resonant oscillation of ν_e\leftrightarrowν_{μ,τ} can take place within the inner high density region of the choked jet progenitor with a heavy envelope, altering the neutrino flavor ratio on its surface to Φ^s_{ν_e}:Φ^s_{ν_μ}:Φ^s_{ν_τ}=5:11:2. Considering vacuum oscillation of these neutrinos on their way to Earth, the final flavor ratio detected on Earth is further modified to either for the large mixing angle solution to the solar neutrino data, or 1:1.3:1.3 for maximal mixing among the muon and tau neutrinos in vacuum.
5 pages, two column, revtex style, to be published in Research in Astronomy and Astrophysics (RAA)
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