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Serious searches for the weakly interacting massive particle (WIMP) have nowbegun. In this context, the most important questions that need to be addressedare: "To what extent can we constrain the WIMP models in the future?" and "Whatwill then be the remaining unexplored regions in the WIMP parameter space foreach of these models?" In our quest to answer these questions, we classify WIMPin terms of quantum number and study each case adopting minimality as a guidingprinciple. As a first step, we study one of the simple cases of the minimalcomposition in the well-tempered fermionic WIMP regime, namely thesinglet-doublets WIMP model. We consider all available constraints from directand indirect searches and also the predicted constraints coming from the nearfuture and the future experiments. We thus obtain the current status, the nearfuture prospects and the future prospects of this model in all its generality.We find that in the future, this model will be constrained almost solely by thefuture direct dark matter detection experiments (as compared to the weakerindirect and collider constraints) and the cosmological (relic density)constraints and will hence be gradually pushed to the corner of thecoannihilation region, if no WIMP signal is detected. Future lepton colliderswill then be useful in exploring this region not constrained by any otherexperiments.

WIMP Dark Matter in a Well-Tempered Regime: A case study on Singlet-Doublets Fermionic WIMP