Discussion Overview
The discussion revolves around the concept of how much mass would need to be added to the Milky Way galaxy for it to become a closed universe, particularly in the context of black holes and cosmological models. Participants explore theoretical implications, assumptions about mass distribution, and the nature of time and space within such frameworks.
Discussion Character
- Exploratory
- Debate/contested
- Conceptual clarification
Main Points Raised
- Some participants question the premise that adding mass to the Milky Way could affect the universe's closure, suggesting that the galaxy is not the universe.
- There is a discussion about the conditions under which the Milky Way could be considered "closed," including the amount of dark matter or energy required and its distribution within the galaxy.
- One participant draws parallels between the experience of being inside a black hole and the nature of universal expansion, suggesting that we might be in a state of free fall through time.
- Concerns are raised about the implications of black hole models, particularly regarding the concepts of homogeneity and isotropy in the universe.
- Some participants express uncertainty about the detectability of added mass and its effects on the galaxy's size and structure.
- There is a debate about whether black holes must rotate and how this affects the properties of the universe if it were inside a black hole.
Areas of Agreement / Disagreement
Participants do not reach a consensus on the questions posed, with multiple competing views and uncertainties remaining regarding the implications of adding mass to the Milky Way and the nature of black holes in cosmological models.
Contextual Notes
Participants highlight limitations in understanding the relationship between mass, black holes, and the universe's structure, particularly regarding the definitions of isotropy and homogeneity. There are unresolved questions about the nature of time and the properties of mass in relation to surrounding mass.