We analyse the signatures at the Large Hadron Collider (LHC) of the scotogenic model, when the lightest Z(2)-odd particle is a singlet fermion and a feebly interacting massive particle (FIMP). We further assume that the singlet fermion constitutes the dark matter and that it is produced in the early Universe via the freeze-in mechanism. The small couplings required to reproduce the observed dark matter abundance translate into decay-lengths for the next-to-lightest Z(2)-odd particle which can be macroscopic, potentially leading to spectacular signatures at the LHC. We characterize the possible signals of the model according to the spectrum of the Z(2)-odd particles and we derive, for each of the cases, bounds on the parameters of the model ...
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 analyse the signatures at the Large Hadron Collider (LHC) of the scotogenic model, when the light...
We analyse the signatures at the Large Hadron Collider (LHC) of the scotogenic model, when the light...
The scotogenic model is one of the simplest scenarios for physics beyond the Standard Model that can...
We present a class of dark matter models, in which the dark matter particle is a feebly interacting ...
The scotogenic model is one of the simplest scenarios for physics beyond the Standard Model that can...
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...
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...
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 analyse the signatures at the Large Hadron Collider (LHC) of the scotogenic model, when the light...
We analyse the signatures at the Large Hadron Collider (LHC) of the scotogenic model, when the light...
The scotogenic model is one of the simplest scenarios for physics beyond the Standard Model that can...
We present a class of dark matter models, in which the dark matter particle is a feebly interacting ...
The scotogenic model is one of the simplest scenarios for physics beyond the Standard Model that can...
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...
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...
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...