  The light neutrino masses are at present most stringently constraint via
cosmological probes. In particular the Planck collaboration reports $ \sum
m_\nu \leq 0.12\,\mathrm{eV}$ at $95\%$ CL within the standard cosmological
model. This is more than one order of magnitude stronger than the one arising
from laboratory searches. The cosmological bound taken at face value excludes a
plethora of neutrino flavour models which can successfully explain the neutrino
oscillation data. The indirect nature of the cosmological bound, however,
allows to relax the bound to up to $ \sum m_\nu \sim 1\,\mathrm{eV}$ if
neutrinos decay on timescales shorter than the age of the Universe, $\tau_\nu
\leq t_U$. We present how a decay of the type $\nu_i\to\nu_4\phi$ can be
realized within general models of the minimal extended seesaw framework. The
idea is then explicitly realized within the context of a $U(1)_{\mu-\tau}$
flavour model.
