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departure from known physics, which might also require modifications to our understanding of huge parts of actuality. The reigning candidate for darkish matter is called a Weakly Interacting Massive Particle or WIMP. These speculative entities usually are not discovered in the Standard Model of particle physics, which describes virtually all particles and forces. WIMPs can be extra much like the ghostly neutrino, besides it might weigh 10 to one hundred instances greater than a proton. (Neutrinos’ actual masses are unknown but they’re far lighter than electrons). Yet darkish matter does work together with strange matter. It displays measurable gravitational effects on massive constructions within the universe such as galaxies and galaxy clusters. Because of this, astronomers are in a position to make maps of the distribution of darkish matter within the universe, although they cannot see it directly. Currently there was no nicely-established declare of dark matter detection from a direct detection experiment, leading as an alternative to robust higher limits on the mass and interaction cross part with nucleons of such dark matter particles. The DAMA/NaI and more recent DAMA/LIBRA experimental collaborations have detected an annual modulation within the price of events in their detectors, which they claim is due to darkish matter. This results from the expectation that as the Earth orbits the Sun, the velocity of the detector relative to the darkish matter halo will vary by a small quantity. This claim is so far unconfirmed and in contradiction with negative results from different experiments corresponding to LUX, SuperCDMS and XENON100. If dark matter is made up of sub-atomic particles, then hundreds of thousands, presumably billions, of such particles must move via each square centimeter of the Earth every second. Many experiments purpose to check this hypothesis. Although WIMPs are popular search candidates, the Axion Dark Matter Experiment searches for axions. Another candidate is heavy hidden sector particles which solely interact with strange matter by way of gravity. Warm dark matter contains particles with an FSL comparable to the size of a protogalaxy. Predictions based mostly on heat dark matter are just like these for chilly dark matter on massive scales, but with much less small-scale density perturbations. This reduces the expected abundance of dwarf galaxies and should lead to lower density of dark matter within the central elements of huge galaxies. Some researchers think about this a greater fit to observations. A problem for this model is

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