https://doi.org/10.1140/epjc/s10052-018-5662-y
Review -
The waning of the WIMP? A review of models, searches, and constraints
1 Max Planck Institut für Kernphysik, Saupfercheckweg 1, 69117, Heidelberg, Germany
2 Laboratoire de Physique Théorique, CNRS, Univ. Paris-Sud, Université Paris-Saclay, 91405, Orsay, France
3 Centre de Physique Théorique, Ecole Polytechnique, CNRS, Université Paris-Saclay, 91128, Palaiseau Cedex, France
4 Department of Physics, University of California, Santa Cruz, 1156 High St, 95060, Santa Cruz, CA, USA
5 Santa Cruz Institute for Particle Physics, Santa Cruz, 1156 High St, 95060, Santa Cruz, CA, USA
Received:
12
November
2017
Accepted:
22
February
2018
Published online: 10 March 2018
Weakly Interacting Massive Particles (WIMPs) are among the best-motivated dark matter candidates. No conclusive signal, despite an extensive search program that combines, often in a complementary way, direct, indirect, and collider probes, has been detected so far. This situation might change in near future due to the advent of one/multi-TON Direct Detection experiments. We thus, find it timely to provide a review of the WIMP paradigm with focus on a few models which can be probed at best by these facilities. Collider and Indirect Detection, nevertheless, will not be neglected when they represent a complementary probe.
A Revision of this article is available online at https://doi.org/10.1140/epjc/s10052-024-13672-y.
© The Author(s) 2018
Open Access
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