Linear stability analysis of collective neutrino oscillations without spurious modes
Taiki Morinaga, Shoichi Yamada

TL;DR
This paper addresses the problem of spurious modes in linear stability analysis of collective neutrino oscillations, proposing polynomial and piecewise linear methods to eliminate unphysical eigenmodes and improve analysis accuracy.
Contribution
The authors identify the origin of spurious modes in discretized linear analysis and introduce polynomial and piecewise linear approximations to remove these unphysical solutions.
Findings
Polynomial approximation recovers branch cut singularities
Piecewise linear approximation effectively removes spurious modes
Method applicable to multi-energy and dispersion relation analyses
Abstract
Collective neutrino oscillations are induced by the presence of neutrinos themselves. As such they are intrinsically nonlinear phenomena and are much more complex than linear counterparts such as the vacuum or MSW oscillations. They obey integro-differential equations, numerical solutions of which are also very challenging. If one focuses on the onset of the collective oscillations, on the other hand, the equations can be linearized and the technique of linear analysis can be employed. Unfortunately, however, it is well known that such an analysis, when applied with discretizations of continuous angular distributions, suffers from the appearance of so-called spurious modes, unphysical eigenmodes of the discretized linear equations. In this paper, we analyze in detail the origin of these unphysical modes and present a simple solution to this annoying problem. We have found that the…
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