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  2. Dark matter - Wikipedia

    en.wikipedia.org/wiki/Dark_matter

    In astronomy, dark matter is an invisible and hypothetical form of matter that does not interact with light or other electromagnetic radiation.Dark matter is implied by gravitational effects which cannot be explained by general relativity unless more matter is present than can be observed.

  3. Dark radiation - Wikipedia

    en.wikipedia.org/wiki/Dark_radiation

    Dark radiation (also dark electromagnetism) [1] is a postulated type of radiation that mediates interactions of dark matter.. By analogy to the way photons mediate electromagnetic interactions between particles in the Standard Model (called baryonic matter in cosmology), dark radiation is proposed to mediate interactions between dark matter particles. [1]

  4. Light dark matter - Wikipedia

    en.wikipedia.org/wiki/Light_dark_matter

    These particles are heavier than warm dark matter and hot dark matter, but are lighter than the traditional forms of cold dark matter, such as Massive Compact Halo Objects (MACHOs). The Lee - Weinberg bound [ 2 ] limits the mass of the favored dark matter candidate, WIMPs, that interact via the weak interaction to ≈ 2 {\displaystyle \approx 2 ...

  5. Void (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Void_(astronomy)

    The model makes it clear to see how the matter-dense regions contract under the collective gravitational force while simultaneously aiding in the expansion of cosmic voids as the matter flees to the walls and filaments. Cosmic voids contain a mix of galaxies and matter that is slightly different than other regions in the universe.

  6. Structure formation - Wikipedia

    en.wikipedia.org/wiki/Structure_formation

    As a result, dark matter begins to collapse into a complex network of dark matter halos well before ordinary matter, which is impeded by pressure forces. Without dark matter, the epoch of galaxy formation would occur substantially later in the universe than is observed. The physics of structure formation in this epoch is particularly simple, as ...

  7. Scientists think they know where the early universe’s dark ...

    www.aol.com/news/scientists-think-know-where...

    We can't see dark matter in space because it doesn't reflect light, but it still exerts a gravitational pull, just like "normal" matter. By accounting for the size of a galaxy and the speed at ...

  8. Lambda-CDM model - Wikipedia

    en.wikipedia.org/wiki/Lambda-CDM_model

    Among these models are many that modify the properties of dark energy or of dark matter over time, interactions between dark energy and dark matter, unified dark energy and matter, other forms of dark radiation like sterile neutrinos, modifications to the properties of gravity, or the modification of the effects of inflation, changes to the ...

  9. Can dark matter be found on earth? New research says ‘maybe’

    www.aol.com/dark-matter-found-earth-research...

    Dark matter makes up 85% of all matter in the Universe, but astronomers have never seen it. The mass which we call dark matter does not give off light, heat, radio waves, or any other form of ...