Monte Carlo Neutrino Oscillations
arXiv:hep-ph/0509356 · doi:10.1103/PhysRevD.73.056003
Abstract
We demonstrate that the effects of matter upon neutrino propagation may be recast as the scattering of the initial neutrino wavefunction. Exchanging the differential, Schrodinger equation for an integral equation for the scattering matrix S permits a Monte Carlo method for the computation of S that removes many of the numerical difficulties associated with direct integration techniques.
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- Oscillation Effects and Time Variation of the Supernova Neutrino Signal
- Phase effects in neutrino conversions during a supernova shock wave
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- Simulating nonlinear neutrino flavor evolution
- Shockwaves in Supernovae: New Implications on the Diffuse Supernova Neutrino Background
- Combining collective, MSW, and turbulence effects in supernova neutrino flavor evolution
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- Neutrino Oscillations Within the Induced Gravitational Collapse Paradigm of Long Gamma-Ray Bursts
- Neutrinos from type Ia supernovae: the deflagration-to-detonation transition scenario
- Untangling supernova-neutrino oscillations with beta-beam data
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- The consequences of large θ_13 for the turbulence signatures in supernova neutrinos
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- Supernova neutrinos and the turbulence power spectrum: point source statistics
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