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- W2280621852 abstract "There is over-whelming evidence that the Universe contains a fraction of dark non-baryonic matter 1 , yet its nature remains elusive. Among the variety of possibilities, weakly interacting massive particles (WIMPs) remain the most compelling vision for dark matter, because they offer a natural explanation of the observed abundance of dark matter which is roughly independent of the detailed thermal history of the Universe. WIMPs are also an interesting candidate because they have large (very roughly weak scale) interactions with ordinary matter, leading to good prospects for their detection by particle physics experiments. Given a specific model containing a dark matter candidate particle, such as the neutralino 2 in a model of supersymmetry with R-parity, or the lightest Kaluza-Klein particle 3 in a model with Universal Extra Dimensions,4 one can make detailed predictions for any observable (such as relic density, direct scattering rate, indirect annihilation rate, or production of a signature at colliders) in terms of the underlying model parameters. However, in the absence of a clear indication as to which model is correct, such predictions are difficult to put together into a coherent picture of the constraints on dark matter and interrelation of the various null searches for its presence." @default.
- W2280621852 created "2016-06-24" @default.
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- W2280621852 date "2012-01-01" @default.
- W2280621852 modified "2023-09-27" @default.
- W2280621852 title "Effective theory descriptions of dark matter interactions" @default.
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