# Supplemental material for "Supernova Neutrino Decoupling Is Altered by Flavor Conversion" (arXiv:2206.00676)

Authors: Shashank Shalgar and Irene Tamborra

In the following animations, the panels on the left show the evolution of $\rho_{ee}$ and $\bar{\rho}_{ee}$ in the plane spanned by $r$ and $\cos\theta$ as functions of the simulation time. The panels on the right display the difference between $\rho_{ee}$ and $\bar{\rho}_{ee}$ with and without flavor transformation. In the initial part of the simulation (first $10^{-4}$ s), flavor conversion is switched off. Once the steady state is reached, we switch on flavor conversion.