Stimulated Neutrino Transformation with Sinusoidal Density Profiles
arXiv:1202.0776 · doi:10.1088/0954-3899/40/5/055002
Abstract
Large amplitude oscillations between the states of a quantum system can be stimulated by sinusoidal external potentials with frequencies that are similar to the energy level splitting of the states or a fraction thereof. Situations when the applied frequency is equal to an integer fraction of the energy level splittings are known as parametric resonances. We investigate this effect for neutrinos both analytically and numerically for the case of arbitrary numbers of neutrino flavors. We look for environments where the effect may be observed and find that supernova are the one realistic possibility due to the necessity of both large densities and large amplitude fluctuations. The comparison of numerical and analytic results of neutrino propagation through a model supernova reveals it is possible to predict the locations and strengths of the stimulated transitions that occur.
14 pages, 6 figures
References in corpus (4)
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- Neutrino Flavour Evolution Through Fluctuating Matter
- Supernova neutrinos and the turbulence power spectrum: point source statistics
- Exact solution to neutrino-plasma two-flavor dynamics
- Matter parametric neutrino flavor transformation through Rabi resonances