Discussion Overview
The discussion explores the possibility of stars and planets being composed entirely of dark matter (DM), including considerations of how such celestial bodies could be detected and the physical principles governing their formation.
Discussion Character
- Debate/contested
- Conceptual clarification
Main Points Raised
- One participant questions the possibility of stars and planets being composed entirely of dark matter, noting uncertainty about the definition of a star based on its fuel.
- Another participant asserts that dark matter cannot lose enough energy to collapse into stars or planets, referencing the concept of early Universe dark stars that are predominantly matter.
- A follow-up question asks how much energy dark matter would need to lose to collapse into celestial bodies.
- Further elaboration suggests that dark matter cannot lose energy through processes like heat transformation, which is necessary for the formation of larger objects from smaller ones.
- One participant emphasizes that if dark matter consists of particles, they cannot combine to form larger structures due to their inability to lose energy.
Areas of Agreement / Disagreement
Participants generally disagree on the feasibility of dark matter forming stars or planets, with multiple competing views regarding the physical properties of dark matter and its ability to collapse into larger celestial bodies.
Contextual Notes
The discussion highlights limitations in understanding the energy dynamics of dark matter and its interactions, particularly regarding its inability to lose energy and the implications for celestial formation.