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  2. Sanford Underground Research Facility - Wikipedia

    en.wikipedia.org/wiki/Sanford_Underground...

    The Davis Cavern gave the experiment the environment it needed to become the most sensitive dark matter detector in the world, a spot it held for more than one year after it was decommissioned. This state-of-the-art laboratory features a 72,000-gallon (272,549 liters) water tank, which serves as additional shielding from cosmic radiation; and a ...

  3. Dark matter - Wikipedia

    en.wikipedia.org/wiki/Dark_matter

    The categories of dark matter are set with respect to the size of a protogalaxy (an object that later evolves into a dwarf galaxy): dark matter particles are classified as cold, warm, or hot if their FSL is much smaller (cold), similar to (warm), or much larger (hot) than a protogalaxy.

  4. Large Underground Xenon experiment - Wikipedia

    en.wikipedia.org/wiki/Large_Underground_Xenon...

    The Large Underground Xenon experiment (LUX) aimed to directly detect weakly interacting massive particle (WIMP) dark matter interactions with ordinary matter on Earth. . Despite the wealth of (gravitational) evidence supporting the existence of non-baryonic dark matter in the Universe, [1] dark matter particles in our galaxy have never been directly detected in an expe

  5. Dark Matter May Not Be Invisible After All. This Discovery ...

    www.aol.com/dark-matter-may-not-invisible...

    Dark matter is called ‘dark’ because it’s invisible to us and does not measurably interact with anything other than gravity. It could be interspersed between the atoms that make up the Earth ...

  6. Stawell Underground Physics Laboratory - Wikipedia

    en.wikipedia.org/wiki/Stawell_Underground...

    The project's Southern Hemisphere location has bearing on the possible differential detection of the putative WIMP-wind.Northern Hemisphere instruments are showing hints of a June "bump" of possible dark matter hits, [7] which is expected given the galaxy's rotation, but it is hard to be sure that it is not a false signal due to some subtle seasonal environmental effect.

  7. LZ experiment - Wikipedia

    en.wikipedia.org/wiki/LZ_experiment

    The two goals of a dark matter search are to minimize the number of these background interactions, and for those that do occur, to be able to identify that they are from background (as opposed to WIMPs). First, the innermost detector is composed of a dual-phase xenon time projection chamber (TPC).

  8. Scientists Built an Ingenious Trap to Catch Dark Matter. We ...

    www.aol.com/scientists-built-ingenious-trap...

    A new experiment underway at the University of Nottingham aims to create a dark matter “trap” that attempts to study domain walls, or dark walls, according to the theory of scalar fields.

  9. DarkSide (dark matter experiment) - Wikipedia

    en.wikipedia.org/wiki/DarkSide_(dark_matter...

    The DarkSide collaboration is an international affiliation of universities and labs seeking to directly detect dark matter in the form of weakly interacting massive particles (WIMPs). The collaboration is planning, building and operating a series of liquid argon time projection chambers (TPCs) that are employed at the Gran Sasso National ...