Dark Matter

Definition of Dark Matter as it relates to Science, Astronomy, Cosmochemistry

Dark Matter is a theoretical form of matter that is believed to make up approximately 85% of the universe's mass. It does not emit, reflect or absorb light, making it extremely difficult to detect and study directly. In cosmochemistry, dark matter is an essential component in understanding the formation and evolution of galaxies, as well as the large-scale structure of the universe. Its presence can be inferred through its gravitational effects on visible matter, such as stars and galaxies. Despite extensive research, dark matter remains one of the most mysterious and intriguing areas of study in cosmochemistry, with ongoing efforts to directly detect it and understand its properties.

Note
  • [dance.rice.edu] October 28th 29th, 2019. DANCE: Dark-matter And Neutrino Computation Explored. | A workshop on the computational aspects (analysis tools, machine learning, distributed computing, data acquisition) of current direct-detection dark matter experiments and medium-sized neutrino experiments.
  • [lz.lbl.gov] The LZ Dark Matter Experiment | The status and science of the LZ dark matter experiment.
  • [darwin.physik.uzh.ch] DARWIN - Dark Matter WIMP Search With Liquid Xenon
  • [xenon1t.org] XENONnT experiment – Direct Search for Dark Matter with Liquid Xenon Deep Underground at the Laboratori Nazionali del Gran Sasso
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