If the annihilation products of dark matter (DM) are non-relativistic and couples directly to a light force mediator, the non-perturbation effect like final state bound state (FBS) formation and final state Sommerfeld (FSS) effect must be considered. Non-relativistic region of final particles will appear when there is small mass split between DM and products, so we study those effects in the degenerate region of mass (including kinematics forbidden case) using two specific models. We demonstrate that FBS effect will significantly modify the DM relic abundance comparing to the standard perturbation calculation in some mass split region. We emphasize that FBS effect is comparable to the FSS effect in those mass split. The conservation angular...
An era of kination occurs when the Universe's energy density is dominated by a fast-rolling scalar f...
Primordial Black Holes (PBH) could dominate in the early universe and, evaporating before Big bang N...
We propose a two-component dark matter explanation to the EDGES 21 cm anomalous signal. The heavier ...
We explore the impact of non-perturbative effects, namely Sommerfeld enhancement and bound state for...
The existence of a dark matter model with a rich dark sector could be the reason why WIMP dark matte...
We explore the impact of highly excited bound states on the evolution of number densities of new phy...
We explore a new mechanism for reproducing the Dark Matter (DM) abundance: scatterings of one DM par...
The formation and decay of metastable bound states can significantly decrease the thermal-relic dark...
A novel particle has been and still is an intriguing option to explain the strong evidence for dark ...
In order to predict the cosmological abundance of dark matter, an estimation of particle rates in an...
We study the impact of bound state formation on dark matter annihilation rates in models where dark ...
We present generic formulæ for computing how Sommerfeld corrections together with bound-state format...
We present generic formulae for computing how bound state formation affects the thermal abundance of...
In many models of dark matter (DM), several production mechanisms contribute to its final abundance,...
In this work, we reanalyze the multi-component strongly interacting massive particle (mSIMP) scenari...
An era of kination occurs when the Universe's energy density is dominated by a fast-rolling scalar f...
Primordial Black Holes (PBH) could dominate in the early universe and, evaporating before Big bang N...
We propose a two-component dark matter explanation to the EDGES 21 cm anomalous signal. The heavier ...
We explore the impact of non-perturbative effects, namely Sommerfeld enhancement and bound state for...
The existence of a dark matter model with a rich dark sector could be the reason why WIMP dark matte...
We explore the impact of highly excited bound states on the evolution of number densities of new phy...
We explore a new mechanism for reproducing the Dark Matter (DM) abundance: scatterings of one DM par...
The formation and decay of metastable bound states can significantly decrease the thermal-relic dark...
A novel particle has been and still is an intriguing option to explain the strong evidence for dark ...
In order to predict the cosmological abundance of dark matter, an estimation of particle rates in an...
We study the impact of bound state formation on dark matter annihilation rates in models where dark ...
We present generic formulæ for computing how Sommerfeld corrections together with bound-state format...
We present generic formulae for computing how bound state formation affects the thermal abundance of...
In many models of dark matter (DM), several production mechanisms contribute to its final abundance,...
In this work, we reanalyze the multi-component strongly interacting massive particle (mSIMP) scenari...
An era of kination occurs when the Universe's energy density is dominated by a fast-rolling scalar f...
Primordial Black Holes (PBH) could dominate in the early universe and, evaporating before Big bang N...
We propose a two-component dark matter explanation to the EDGES 21 cm anomalous signal. The heavier ...