Discussion Overview
The discussion revolves around Justin Khoury's hypothesis that dark matter can be modeled as a superfluid, potentially explaining MOND (Modified Newtonian Dynamics) on galactic scales. Participants explore the implications of scaling invariance in this context, particularly its relation to Milgrom's work and the Tully-Fisher relation. The scope includes theoretical considerations, conceptual clarifications, and comparisons of different models.
Discussion Character
- Exploratory
- Technical explanation
- Conceptual clarification
- Debate/contested
Main Points Raised
- Some participants question the connection between Khoury's superfluid model and Milgrom's scaling invariance, noting that Khoury does not explicitly mention scaling invariance in his work.
- Others suggest that the correlation length in a superfluid could imply a phase transition leading to scale invariance, which might relate to Milgrom's emergent symmetry in MOND.
- A participant points out that MOND is not manifestly scale invariant due to its fundamental parameter, but it may exhibit scale invariance in the deep-MOND regime.
- Some argue that more connections need to be established between Khoury's and Milgrom's theories to clarify their relationship.
- There is mention of other models that claim to reproduce MOND phenomenology and whether they exhibit scaling invariance under certain conditions.
- A participant discusses their own research on gravity theories and the implications of scaling symmetries, suggesting that Milgrom's comments could lead to new symmetry algebras.
Areas of Agreement / Disagreement
Participants express differing views on the relationship between Khoury's superfluid model and Milgrom's scaling invariance. There is no consensus on whether these concepts are connected or how they might relate to each other.
Contextual Notes
Some participants highlight the need for further exploration of the connections between different theoretical frameworks and the implications of scaling symmetries, indicating that the discussion is still in a speculative phase.