We calculate the post-recombination contribution to the Cosmic Microwave Background (CMB) spectral distortion due to general exotic energy injections, including dark matter (DM) decaying or annihilating to Standard Model particles. Upon subtracting the background distortion that would be present even without such energy injections, we find residual distortions that are still potentially large enough to be detectable by future experiments such as PIXIE. The distortions also have a high-energy spectral feature that is a unique signature of the injection of high-energy particles. We present a calculation of the global ionization history in the presence of decaying dark matter with sub-keV masses, and also show that previous calculations of the...
The presence of light thermally coupled dark matter affects early expansion history and production o...
International audienceFollowing the pioneering observations with COBE in the early 1990s, studies of...
We use the latest cosmic microwave background (CMB) observations to provide updated constraints on t...
Decaying or annihilating dark matter and other exotic energy injections can modify the spectrum of t...
International audienceWe compute cosmic microwave background (CMB) anisotropy constraints on exoticf...
We compute in detail the rate at which energy injected by dark matter annihilation heats and ionizes...
Any injection of electromagnetically interacting particles during the cosmic dark ages will lead to ...
We consider particle decays during the cosmic dark ages with two aims: (1) to explain the high optic...
If dark matter decays to electromagnetically interacting particles, it can inject energy into the ba...
Cosmic microwave background (CMB) constraints on dark matter annihilation are a uniquely powerful to...
If dark matter resides in a hidden sector minimally coupled to the Standard Model, another particle ...
The radiation background produced by the 21 cm spin-flip transition of neutral hydrogen at high reds...
International audienceFollowing the pioneering observations with COBE in the early 1990s, studies of...
The early universe may have contained internally thermalized dark sectors that were decoupled from t...
The presence of light thermally coupled dark matter affects early expansion history and production o...
International audienceFollowing the pioneering observations with COBE in the early 1990s, studies of...
We use the latest cosmic microwave background (CMB) observations to provide updated constraints on t...
Decaying or annihilating dark matter and other exotic energy injections can modify the spectrum of t...
International audienceWe compute cosmic microwave background (CMB) anisotropy constraints on exoticf...
We compute in detail the rate at which energy injected by dark matter annihilation heats and ionizes...
Any injection of electromagnetically interacting particles during the cosmic dark ages will lead to ...
We consider particle decays during the cosmic dark ages with two aims: (1) to explain the high optic...
If dark matter decays to electromagnetically interacting particles, it can inject energy into the ba...
Cosmic microwave background (CMB) constraints on dark matter annihilation are a uniquely powerful to...
If dark matter resides in a hidden sector minimally coupled to the Standard Model, another particle ...
The radiation background produced by the 21 cm spin-flip transition of neutral hydrogen at high reds...
International audienceFollowing the pioneering observations with COBE in the early 1990s, studies of...
The early universe may have contained internally thermalized dark sectors that were decoupled from t...
The presence of light thermally coupled dark matter affects early expansion history and production o...
International audienceFollowing the pioneering observations with COBE in the early 1990s, studies of...
We use the latest cosmic microwave background (CMB) observations to provide updated constraints on t...