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Direct detection of dark matter is the science of attempting to directly measure dark matter collisions in Earth-based experiments. Modern astrophysical measurements, such as from the Cosmic Microwave Background, strongly indicate that 85% of the matter content of the universe is unaccounted for. Although the existence of dark matter is widely believed, what form it takes or its precise properties has never been determined. There are three main avenues of research to detect dark matter: attempts to make dark matter in accelerators, indirect detection of dark matter annihilation, and direct detection of dark matter in terrestrial labs. The founding principle of direct dark matter detection is that since dark matter is known to exist in the local universe, as the Earth, Solar System, and the Milky Way Galaxy carve out a path through the universe they must intercept dark matter, regardless of what form it takes.
References
- ↑ Macpherson, Alick L.; Pinfold, James L. (1994). "Fermi Ball Detection". arXiv: hep-ph/9412264 .
- ↑ Kawana, Kiyoharu; Xie, Ke-Pan (January 2022). "Primordial black holes from a cosmic phase transition: The collapse of Fermi-balls". Physics Letters B. 824: 136791. arXiv: 2106.00111 . doi:10.1016/j.physletb.2021.136791.
- ↑ Kawana, Kiyoharu; Xie, Ke-Pan (2022). "Primordial black holes from a cosmic phase transition: The collapse of Fermi-balls". Physics Letters B. 824. arXiv: 2106.00111 . Bibcode:2022PhLB..82436791K. doi:10.1016/j.physletb.2021.136791.
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