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In cosmology and physics, cold dark matter (CDM) is a hypothetical type of dark matter. According to the current standard model of cosmology, the Lambda-CDM model, approximately 27% of the universe is dark matter and 68% is dark energy, with only a small fraction being the ordinary baryonic matter that composes stars, planets, and living organisms.
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dark matter galaxies cold model massive axions particles galaxy universe stars observed small cdm weakly structure problem dwarf theory observations
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| black holes | instance of | condensed objects | 0.80 | text |
| neutron stars | instance of | condensed objects | 0.80 | text |
| white dwarfs | instance of | condensed objects | 0.80 | text |
| very faint stars | instance of | condensed objects | 0.80 | text |
| or non-luminous objects like planets | instance of | condensed objects | 0.80 | text |
| Cold dark matter | related to Challenges | Several | 0.60 | section |
| Cold dark matter | related to Challenges | Some | 0.60 | section |
| Cold dark matter | related to Composition | Dark | 0.60 | section |
| Cold dark matter | related to Composition | As | 0.60 | section |
| Cold dark matter | related to Composition | The | 0.60 | section |
| Cold dark matter | related to Composition | Axions | 0.60 | section |
| Cold dark matter | related to Composition | CDM | 0.60 | section |
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