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Fuzzy cold dark matter is a hypothetical form of cold dark matter proposed to solve the cuspy halo problem. It would consist of extremely light scalar particles with masses on the order of eV; so a Compton wavelength on the order of 1 light year. Fuzzy cold dark matter halos in dwarf galaxies would manifest wave behavior on astrophysical scales, and the cusps would be avoided through the Heisenberg uncertainty principle.The wave behavior leads to interference patterns, spherical soliton cores in dark matter halo centers, and cylindrical soliton-like cores in dark matter cosmic web filaments.

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  • Materi gelap dingin samar (in)
  • Fuzzy cold dark matter (en)
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  • Materi gelap dingin samar adalah sebuah bentuk hipotetis yang diusulkan untuk memecahkan . Materi gelap ini kemungkinan terdiri dari partikel skalar yang sangat ringan dengan massa sesuai urutan eV. Halo materi gelap dingin samar di galaksi kerdil akan memanifestasikan perilaku gelombang pada skala astrofisika, dan katupnya akan dihindari melalui prinsip ketidakpastian Heisenberg. Materi gelap dingin samar adalah batas tanpa swa-interaksi. (in)
  • Fuzzy cold dark matter is a hypothetical form of cold dark matter proposed to solve the cuspy halo problem. It would consist of extremely light scalar particles with masses on the order of eV; so a Compton wavelength on the order of 1 light year. Fuzzy cold dark matter halos in dwarf galaxies would manifest wave behavior on astrophysical scales, and the cusps would be avoided through the Heisenberg uncertainty principle.The wave behavior leads to interference patterns, spherical soliton cores in dark matter halo centers, and cylindrical soliton-like cores in dark matter cosmic web filaments. (en)
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  • Fuzzy cold dark matter is a hypothetical form of cold dark matter proposed to solve the cuspy halo problem. It would consist of extremely light scalar particles with masses on the order of eV; so a Compton wavelength on the order of 1 light year. Fuzzy cold dark matter halos in dwarf galaxies would manifest wave behavior on astrophysical scales, and the cusps would be avoided through the Heisenberg uncertainty principle.The wave behavior leads to interference patterns, spherical soliton cores in dark matter halo centers, and cylindrical soliton-like cores in dark matter cosmic web filaments. Fuzzy cold dark matter is a limit of scalar field dark matter without self-interaction. It is governed by the Schrödinger–Poisson equation. (en)
  • Materi gelap dingin samar adalah sebuah bentuk hipotetis yang diusulkan untuk memecahkan . Materi gelap ini kemungkinan terdiri dari partikel skalar yang sangat ringan dengan massa sesuai urutan eV. Halo materi gelap dingin samar di galaksi kerdil akan memanifestasikan perilaku gelombang pada skala astrofisika, dan katupnya akan dihindari melalui prinsip ketidakpastian Heisenberg. Materi gelap dingin samar adalah batas tanpa swa-interaksi. (in)
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