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these outcomes are constant, it would even be nice to have an analogous accounting of strange matter at present. dashing up, and never slowing down as anticipated. This result implies the existence of large amounts of “darkish energy” whose gravitational pressure is repulsive (see Box 5.1). Maps of the long filaments of gasoline that hold the universe together may one day assist us hint and unveil ‘darkish matter’. A current experiment with atomic nuclei is tough to sq. with our current understanding of physics. A new method suggests we should purpose to detect dark matter haloes by tracing galactic fuel. Researchers have discovered a approach to velocity up the seek for dark matter using technology from quantum computing. By squeezing quantum noise, detectors can now look for axions twice as fast. Plus new research finds a method to pace up the seek for dark matter. Listen to episode four of The Conversation Weekly. Because neutrinos are so weakly interacting, neutrino telescopes should be massive to detect a major signal. AMANDA-II is a neutrino detector 1500 to 2000 meters underground within the ice of the South Pole the place Cherenkov radiation can journey and be seen simply by optical modules. This experiment has not detected statistically significant results from the path of the Sun, but has placed helped place agency limits on the muon flux . A future experiment , IceCube, will combine AMANDA into a a lot bigger detection experiment, with 7200 optical modules and a detector quantity of a cubic kilometer . Super-Kamiokande (“Super-K”) is one other oblique detection experiment, located underground in the Kamioka-Mozumi mine in Japan. The detector consists of 50,000 tons of water and detects Cherenkov radiation from incoming muons as well. Super-K looks in the direction of the Sun, earth, and galactic middle, and, like AMANDA, has not detected any extra of muon charges above the expected background . While many others are in operation worldwide, the three direct detection experiments which have yielded one of the best results for the spin-independent WIMP-nucleus cross part are the Cryogenic Dark Matter Search within the Soudan Mine, the UK Dark Matter Collaboration’s ZEPLIN-I within the Boulby Mine, and XENON10 on the Gran Sasso Underground Laboratory. where is the whole mass of nuclei of species within the detector that has been energetic for a time , and is the counting effectivity for nuclear

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