Fetching the paper…
Reading the bibliography…
Models in which the dark matter is very weakly coupled to the observable sector may explain the observed dark matter density, either as a "superWIMP" or as "asymmetric dark matter." Both types of models predict displaced vertices at colliders, with a rich variety of possible phenomenology.
Nothing clear enough to list yet.
Nothing clear enough to list yet.
Nothing clear enough to list yet.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…