We explore the impact of non-perturbative effects, namely Sommerfeld enhancement and bound state formation, on the cosmological production of non-thermal dark matter. For this purpose, we focus on a class of simplified models with t-channel mediators. These naturally combine the requirements for large corrections in the early Universe, i.e. beyond the Standard Model states with long range interactions, with a sizable new physics production cross section at the LHC. We find that the dark matter yield of the superWIMP mechanism is suppressed considerably due to the non-perturbative effects under consideration. This leads to a significant shift in the cosmologically preferred parameter space of non-thermal dark matter in these models. We also ...
We present generic formulae for computing how bound state formation affects the thermal abundance of...
We present generic formulæ for computing how Sommerfeld corrections together with bound-state forma...
We describe the evolution of Dark Matter (DM) abundance from the very onset of its creation from inf...
We explore the impact of highly excited bound states on the evolution of number densities of new phy...
The existence of a dark matter model with a rich dark sector could be the reason why WIMP dark matte...
A novel particle has been and still is an intriguing option to explain the strong evidence for dark ...
If the annihilation products of dark matter (DM) are non-relativistic and couples directly to a ligh...
Non-thermalized dark matter is a cosmologically viable alternative to the widely studied weakly inte...
In order to predict the cosmological abundance of dark matter, an estimation of particle rates in an...
We explore a new mechanism for reproducing the Dark Matter (DM) abundance: scatterings of one DM par...
In many models of dark matter (DM), several production mechanisms contribute to its final abundance,...
We present generic formulæ for computing how Sommerfeld corrections together with bound-state format...
The formation and decay of metastable bound states can significantly decrease the thermal-relic dark...
Within the Minimal Supersymmetric Standard Model (MSSM), LHC bounds suggest that scalar superpartner...
Recently many investigations have considered Majorana dark matter co-annihilating with bound states ...
We present generic formulae for computing how bound state formation affects the thermal abundance of...
We present generic formulæ for computing how Sommerfeld corrections together with bound-state forma...
We describe the evolution of Dark Matter (DM) abundance from the very onset of its creation from inf...
We explore the impact of highly excited bound states on the evolution of number densities of new phy...
The existence of a dark matter model with a rich dark sector could be the reason why WIMP dark matte...
A novel particle has been and still is an intriguing option to explain the strong evidence for dark ...
If the annihilation products of dark matter (DM) are non-relativistic and couples directly to a ligh...
Non-thermalized dark matter is a cosmologically viable alternative to the widely studied weakly inte...
In order to predict the cosmological abundance of dark matter, an estimation of particle rates in an...
We explore a new mechanism for reproducing the Dark Matter (DM) abundance: scatterings of one DM par...
In many models of dark matter (DM), several production mechanisms contribute to its final abundance,...
We present generic formulæ for computing how Sommerfeld corrections together with bound-state format...
The formation and decay of metastable bound states can significantly decrease the thermal-relic dark...
Within the Minimal Supersymmetric Standard Model (MSSM), LHC bounds suggest that scalar superpartner...
Recently many investigations have considered Majorana dark matter co-annihilating with bound states ...
We present generic formulae for computing how bound state formation affects the thermal abundance of...
We present generic formulæ for computing how Sommerfeld corrections together with bound-state forma...
We describe the evolution of Dark Matter (DM) abundance from the very onset of its creation from inf...