Discussion Overview
The discussion revolves around the hypothesis that cold dark matter might be composed of ice or water vapor. Participants explore the implications of this idea in relation to the known baryonic content of the universe, the nature of dark matter, and its gravitational effects.
Discussion Character
- Debate/contested
- Exploratory
- Technical explanation
Main Points Raised
- One participant suggests that cold dark matter could be ice, linking it to the abundance of water created since the universe's formation.
- Another participant counters that cold dark matter does not interact with electromagnetic radiation, unlike water, which emits and absorbs light.
- A participant elaborates on the baryonic content of the universe, noting that while water is a common compound, its contribution to the total mass is minimal, suggesting that dark matter cannot be primarily water.
- Some participants express curiosity about the possibility of baryonic matter existing in forms that do not interact with electromagnetic radiation, questioning the assumptions about dark matter's composition.
- One participant mentions evidence of black holes emitting trace amounts of water vapor, proposing that dark matter could be dispersed water vapor that is currently unmeasurable.
- Another participant emphasizes that for dark matter to exert its gravitational influence, it must exist in large quantities, which would imply observable effects if it were composed of gaseous matter.
Areas of Agreement / Disagreement
Participants express differing views on the nature of dark matter, with some supporting the idea that it could be water or ice, while others argue against this hypothesis based on the known properties of dark matter. The discussion remains unresolved, with multiple competing views present.
Contextual Notes
Participants highlight limitations in current understanding, such as the difficulty in measuring certain forms of matter and the assumptions underlying the nature of dark matter. The discussion reflects ongoing uncertainties in cosmological models.