review Open AccessTop 1% cited
The waning of the WIMP? A review of models, searches, and constraints
The European Physical Journal C · 2018 · Vol. 78(3) · pp. 203–203
Giorgio Arcadi✉(Max Planck Institute for Nuclear Physics)Maíra Dutra(Laboratoire de Physique Théorique)Pradipta Ghosh(Laboratoire de Physique Théorique)M. Lindner(Max Planck Institute for Nuclear Physics)Yann Mambrini(Université Paris-Sud)Mathias Pierre(Université Paris-Saclay)Stefano Profumo(University of California, Santa Cruz)Farinaldo S. Queiroz(Max Planck Institute for Nuclear Physics)
Abstract
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.
Dark Matter and Cosmic PhenomenaParticle physics theoretical and experimental studiesParticle Detector Development and PerformanceWIMPWeakly interacting massive particlesDark matterColliderPhysicsFocus (optics)Particle physicsAstronomyCosmologyDark energy
Funding
- U.S. Department of Energy
- European Commission
- Conselho Nacional de Desenvolvimento Científico e Tecnológico
- Centre National de la Recherche Scientifique
- Ministerio de Ciencia e Innovación
- Research Executive Agency
- Ciência sem Fronteiras
Citations
858
FWCI
171.43
field-weighted impact
References
403
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100%
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