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Despite compelling arguments that significant discoveries of physics beyondthe standard model are likely to be made at the Large Hadron Collider, itremains possible that this machine will make no such discoveries, or will makeno discoveries directly relevant to the dark matter problem. In this article,we study the ability of astrophysical experiments to deduce the nature of darkmatter in such a scenario. In most dark matter studies, the relic abundance anddetection prospects are evaluated within the context of some specific particlephysics model or models (e.g. supersymmetry). Here, we attempt to develop amodel-independent approach toward the phenomenology of weakly interactingmassive particles in the absence of any discoveries at the Large HadronCollider. In particular, we consider generic fermionic or scalar dark matterparticles with a variety of interaction forms, and calculate the correspondingconstraints from and sensitivity of direct and indirect detection experiments.The results may provide some guidance in disentangling information from futuredirect and indirect detection experiments.

Deducing the nature of dark matter from direct and indirect detection experiments in the absence of collider signatures of new physics