2018
DOI: 10.1140/epjc/s10052-018-5662-y
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The waning of the WIMP? A review of models, searches, and constraints

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. … Show more

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Cited by 802 publications
(805 citation statements)
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References 350 publications
(564 reference statements)
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“…Furthermore, one finds in the 4-D case that an additional problem arises if M DM > M DP . If this occurs the DM can annihilate into pairs of DPs which is found to be an s-wave process for both fermionic and bosonic DM in the initial state [1] and is thus constrained by the CMB. In the 5-D case, this tells us that the lightest mode in the DM KK tower (i.e., the actual DM) must be lighter than the corresponding lightest KK state in the DP mediator tower which can be a significant model-building constraint.…”
Section: Cosmology: Planck and Cmb Constraintsmentioning
confidence: 99%
“…Furthermore, one finds in the 4-D case that an additional problem arises if M DM > M DP . If this occurs the DM can annihilate into pairs of DPs which is found to be an s-wave process for both fermionic and bosonic DM in the initial state [1] and is thus constrained by the CMB. In the 5-D case, this tells us that the lightest mode in the DM KK tower (i.e., the actual DM) must be lighter than the corresponding lightest KK state in the DP mediator tower which can be a significant model-building constraint.…”
Section: Cosmology: Planck and Cmb Constraintsmentioning
confidence: 99%
“…The upper bounds on the cross section off the nucleon is obtained by LUX [102] and XENON1T [103]. In the cases of onecomponent DM system of a real or complex scalar boson, those experimental results give the strong constraint on the masses of those DM particles; the allowed DM mass region is ≃m h /2 and > ∼ 1 TeV [104][105][106]. In the model A with the multicomponent DM system, the constrains on the cross sections off the nucleon for χ and φ R are also relatively severe.…”
Section: Multicomponent Dark Matter Systemmentioning
confidence: 99%
“…Weakly Interacting Massive Particle (WIMP) [49] is a promising dark matter candidate, since the observed relic density can be naturally derived for a WIMP mass around the electroweak scale. In the U (1) R model, the lightest righthanded Majorana neutrino can be cold dark matter candidate, stabilized by the Z 2 symmetry.…”
Section: Dark Mattermentioning
confidence: 99%