Cosmological decay of Higgs-like scalars into a fermion channel
  We study the decay of a Higgs-like scalar Yukawa coupled to massless fermions
in post-inflationary cosmology, combining a non-perturbative method with an
adiabatic expansion. The renormalized survival probability
$\mathcal{P}_\Phi(t)$ of a (quasi) particle ``born'' at time $t_b$ and decaying
at rest in the comoving frame, $\mathcal{P}_\Phi(t) =
\Big[\frac{t}{t_b}\Big]^{-\frac{Y^2}{8\pi^2}}~ e^{
\frac{Y^2}{4\pi^2}\,\big(t/t_b\big)^{1/4} } \,e^{-\Gamma_0\,(t-t_b)}~
\mathcal{P}_\Phi(t_b) $, with $\Gamma_0$ the decay rate at rest in Minkowski
space-time. For an ultrarelativistic particle we find $\mathcal{P}_\Phi(t) =
e^{-\frac{2}{3}\Gamma_0\,t_{nr}\,(t/t_{nr})^{3/2}}~ \mathcal{P}_\Phi(t_b)$
before it becomes non-relativistic at a time $t_{nr}$ as a consequence of the
cosmological redshift. For $t\gg t_{nr}$ we find $\mathcal{P}_\Phi(t) =
\Big[\frac{t}{t_{nr}}\Big]^{-\frac{Y^2}{8\pi^2}}~ e^{
\frac{Y^2}{4\pi^2}\,\big(t/t_{nr}\big)^{1/4}
}~\Big[\frac{t}{t_{nr}}\Big]^{\Gamma_0 t_{nr}/2} \,e^{-\Gamma_0\,(t-t_{nr})}~
\mathcal{P}_\Phi(t_{nr})$. The extra power is a consequence of the memory on
the past history of the decay process. We compare these results to an S-matrix
inspired phenomenological Minkowski-like decay law modified by an instantaneous
Lorentz factor to account for cosmological redshift. Such phenomenological
description \emph{under estimates the lifetime of the particle}. For very long
lived, very weakly coupled particles, we obtain an \emph{upper bound} for the
survival probability as a function of redshift $z$ valid throughout the
expansion history $\mathcal{P}_\Phi(z) \gtrsim
e^{-\frac{\Gamma_0}{H_0}\,\Upsilon(z,z_b)}\,\mathcal{P}_\Phi(z_b)$, where
$\Upsilon(z,z_b)$ only depends on cosmological parameters and $t_{nr}$.
