Cosmological decay of Higgs-like scalars into a fermion channel

Abstract

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 $\mathcal{P}_Φ(t)$ of a (quasi) particle ``born'' at time $t_b$ and decaying at rest in the comoving frame, $\mathcal{P}_Φ(t) = \Big[\frac{t}{t_b}\Big]^{-\frac{Y^2}{8π^2}}~ e^{ \frac{Y^2}{4π^2}\,\big(t/t_b\big)^{1/4} } \,e^{-Γ_0\,(t-t_b)}~ \mathcal{P}_Φ(t_b) $, with $Γ_0$ the decay rate at rest in Minkowski space-time. For an ultrarelativistic particle we find $\mathcal{P}_Φ(t) = e^{-\frac{2}{3}Γ_0\,t_{nr}\,(t/t_{nr})^{3/2}}~ \mathcal{P}_Φ(t_b)$ before it becomes non-relativistic at a time $t_{nr}$ as a consequence of the cosmological redshift. For $t\gg t_{nr}$ we find $\mathcal{P}_Φ(t) = \Big[\frac{t}{t_{nr}}\Big]^{-\frac{Y^2}{8π^2}}~ e^{ \frac{Y^2}{4π^2}\,\big(t/t_{nr}\big)^{1/4} }~\Big[\frac{t}{t_{nr}}\Big]^{Γ_0 t_{nr}/2} \,e^{-Γ_0\,(t-t_{nr})}~ \mathcal{P}_Φ(t_{nr})$. 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 $\mathcal{P}_Φ(z) \gtrsim e^{-\frac{Γ_0}{H_0}\,Υ(z,z_b)}\,\mathcal{P}_Φ(z_b)$, where $Υ(z,z_b)$ only depends on cosmological parameters and $t_{nr}$.