We consider a dark sector consisting of dark matter that is a Dirac fermion and a scalar mediator. This model has been extensively studied in the past. If the scalar couples to the dark matter in a parity conserving manner then dark matter annihilation to two mediators is dominated by the P-wave channel and hence is suppressed at very low momentum. The indirect detection constraint from the anisotropy of the Cosmic Microwave Background is usually thought to be absent in the model because of this suppression. In this letter we show that dark matter annihilation via bound state formation occurs through the S-wave and hence there is a constraint on the parameter space of the model from the Cosmic Microwave Background
Cosmology may give rise to appreciable populations of both particle dark matter and primordial black...
Updated constraints on the dark matter cross section and mass are presented combining cosmic microwa...
The injection of secondary particles produced by dark matter (DM) annihilation around redshift simil...
We consider a dark sector consisting of dark matter that is a Dirac fermion and a scalar mediator. T...
We consider a dark sector consisting of dark matter that is a Dirac fermion and a scalar mediator. T...
We use the latest cosmic microwave background (CMB) observations to provide updated constraints on t...
Precise measurements of the temperature and polarization anisotropies of the cosmic microwave backgr...
Recent measurements of the cosmic microwave background (CMB) anisotropies by Planck provide a sensit...
We compute the bounds on the dark matter (DM) annihilation cross section using the most recent Cosmi...
AbstractHints of direct dark matter detection coming from the DAMA, CoGeNT experiments point toward ...
Cosmic microwave background (CMB) constraints on dark matter annihilation are a uniquely powerful to...
The thermal relic density of dark matter is conventionally set by two-body annihilations. We point o...
We study the impact of bound state formation on dark matter annihilation rates in models where dark ...
If dark matter decays to electromagnetically interacting particles, it can inject energy into the ba...
AbstractLight fermionic/scalar dark matter (DM) (mDM≈8 GeV) neutral under the standard model can be ...
Cosmology may give rise to appreciable populations of both particle dark matter and primordial black...
Updated constraints on the dark matter cross section and mass are presented combining cosmic microwa...
The injection of secondary particles produced by dark matter (DM) annihilation around redshift simil...
We consider a dark sector consisting of dark matter that is a Dirac fermion and a scalar mediator. T...
We consider a dark sector consisting of dark matter that is a Dirac fermion and a scalar mediator. T...
We use the latest cosmic microwave background (CMB) observations to provide updated constraints on t...
Precise measurements of the temperature and polarization anisotropies of the cosmic microwave backgr...
Recent measurements of the cosmic microwave background (CMB) anisotropies by Planck provide a sensit...
We compute the bounds on the dark matter (DM) annihilation cross section using the most recent Cosmi...
AbstractHints of direct dark matter detection coming from the DAMA, CoGeNT experiments point toward ...
Cosmic microwave background (CMB) constraints on dark matter annihilation are a uniquely powerful to...
The thermal relic density of dark matter is conventionally set by two-body annihilations. We point o...
We study the impact of bound state formation on dark matter annihilation rates in models where dark ...
If dark matter decays to electromagnetically interacting particles, it can inject energy into the ba...
AbstractLight fermionic/scalar dark matter (DM) (mDM≈8 GeV) neutral under the standard model can be ...
Cosmology may give rise to appreciable populations of both particle dark matter and primordial black...
Updated constraints on the dark matter cross section and mass are presented combining cosmic microwa...
The injection of secondary particles produced by dark matter (DM) annihilation around redshift simil...