baryonic dark matter mâde-ye siyâh-e bâriyoni Fr.: matière noire baryonique → Dark matter made up of → baryons that are not luminous enough to produce any detectable radiation. It is generally believed that most dark matter is → non-baryonic. The baryonic dark matter could reside in a number of forms, including cold gas and compact objects. |
cold dark matter (CDM) mâdde-ye sard-e târik (#) Fr.: matière noire froide Any → hypothetical → non-baryonic → dark matter that is → non-relativistic at the point of → decoupling in the → early Universe. CDM plays a key role in → cosmic structure formation. See also → CDM model, → lambda cold dark matter, → Meszaros effect, → missing satellites problem. |
hot dark matter mâdde-ye târik-e dâq (#) Fr.: matière noire chaude Any form of → dark matter which had a significant velocity dispersion (comparable to the velocity of light), when the Universe first became → matter-dominated. |
lambda cold dark matter model model-e lâmbdâ-mâde-ye-sard-e-târik Fr.: modèle ΛCDM The → standard model of → Big Bang that incorporates both → dark matter and → dark energy. See also → cold dark matter (CDM). → lambda, → cosmological constant; → cold; → dark; → matter; → model. |
non-baryonic dark matter mâde-ye siyâh-e nâbâriyoni Fr.: matière noire non-baryonique → Dark matter composed of → non-baryonic particles. |