Abstract

We present a numerical survey of the nonlinear flavor development of dense neutrino gases. This study is based on the stationary, two-dimensional ($x$ and $z$), two-beam, monochromatic neutrino line model with a periodic boundary condition along the $x$ direction. Similar to a previous work, we find that small-scale flavor structures can develop in a neutrino gas even if the physical conditions are nearly homogeneous along the $x$ axis initially. The power diffusion from the large-scale to small-scale structures increases with the neutrino density and helps to establish a semi-exponential dependence of the magnitudes of the Fourier moments on the corresponding wave numbers. The overall flavor conversion probabilities in the neutrino gases with small initial sinusoidal perturbations reach certain equilibrium values at large distances which are mainly determined by the neutrino-antineutrino asymmetry. Similar phenomena also exist in a neutrino gas with a localized initial perturbation, albeit only inside an expanding flavor conversion region. Our work suggests that a statistical treatment may be possible for the collective flavor oscillations of a dense neutrino gas in a multi-dimensional environment.

Highlights

  • Because of the mismatch between its weak-interaction and vacuum states, a neutrino can experience flavor transformation or oscillations even in vacuum

  • Similar to a previous work, we find that small-scale flavor structures can develop in a neutrino gas even if the physical conditions are nearly homogeneous along the x axis initially

  • Following the pilot study in Ref. [20] that features a single parameter set (η 1⁄4 þ1, α ≈ 0.77, and μ 1⁄4 13), we have conducted a numerical survey of the two-beam neutrino line model for a wide range of the parameter space.We present a representative collection of our numerical results

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Summary

INTRODUCTION

Because of the mismatch between its weak-interaction and vacuum (mass) states, a neutrino can experience flavor transformation or oscillations even in vacuum (see, e.g., Ref. [1] for a review). Model has been employed to study the neutrino oscillations in the early universe (e.g., [8,9]), and the stationary, spherical neutrino bulb model was used to study the neutrino flavor transformation in supernovae (e.g., [10,11]). In this work we presented a numerical survey on the inhomogeneous, nonlinear flavor transformation of dense neutrino gases.

THE NEUTRINO LINE MODEL
Equations of motion
The flavor pendulum
Spontaneous symmetry breaking
NUMERICAL RESULTS
Numerical method and validation
Sinusoidal initial perturbations
Localized perturbations
CONCLUSIONS

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