Neutrino Flavor Ratios Modified by Cosmic Ray Secondary Acceleration
arXiv:1504.03417 · doi:10.1103/PhysRevD.92.085047
Abstract
Acceleration of 's and 's modifies the flavor ratio at Earth (at astrophysical sources) of neutrinos produced by decay, , from () to () at high energy, because 's decay more than 's during secondary-acceleration. The neutrino spectrum accompanies a flat excess, differently from the case of energy losses. With the flavor spectra, we can probe timescales of cosmic-ray acceleration and shock dynamics. We obtain general solutions of convection-diffusion equations and apply to gamma-ray bursts, which may have the flavor modification at around PeV -- EeV detectable by IceCube and next-generation experiments.
17 pages, 5 figures, accepted for publication in Physical Review D
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- Using High-Energy Neutrinos As Cosmic Magnetometers
- IceCube Flavor Ratios with Identified Astrophysical Sources: Towards Improving New Physics Testability
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- Signatures of secondary acceleration in neutrino flares
- Little Red Dots as Hidden Neutrino Sources
- No Flavor Anisotropy in the High-Energy Neutrino Sky Upholds Lorentz Invariance