We propose simple freeze-in models where the observed dark matter abundance is explained via the decay of an electrically charged and/or coloured parent particle into Feebly Interacting Massive Particles (FIMP). The parent particle is long-lived and yields a wide variety of LHC signatures depending on its lifetime and quantum numbers. We assess the current constraints and future high luminosity reach of these scenarios at the LHC from searches for heavy stable charged particles, disappearing tracks, displaced vertices and displaced leptons. We show that the LHC constitutes a powerful probe of freeze-in dark matter and can further provide interesting insights on the validity of vanilla baryogenesis and leptogenesis scenario
International audienceWe present a class of dark matter models, in which the dark matter particle is...
International audienceWe present a class of dark matter models, in which the dark matter particle is...
International audienceWe present a class of dark matter models, in which the dark matter particle is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
Abstract We propose simple freeze-in models where the observed dark matter abundance is explained vi...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
We present a class of dark matter models, in which the dark matter particle is a feebly interacting ...
International audienceWe present a class of dark matter models, in which the dark matter particle is...
International audienceWe present a class of dark matter models, in which the dark matter particle is...
International audienceWe present a class of dark matter models, in which the dark matter particle is...
International audienceWe present a class of dark matter models, in which the dark matter particle is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
Abstract We propose simple freeze-in models where the observed dark matter abundance is explained vi...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
International audienceWe propose simple freeze-in models where the observed dark matter abundance is...
We present a class of dark matter models, in which the dark matter particle is a feebly interacting ...
International audienceWe present a class of dark matter models, in which the dark matter particle is...
International audienceWe present a class of dark matter models, in which the dark matter particle is...
International audienceWe present a class of dark matter models, in which the dark matter particle is...
International audienceWe present a class of dark matter models, in which the dark matter particle is...