Discussion Overview
The discussion revolves around the definition of the volume form on Riemannian manifolds without relying on local coordinates. Participants explore the possibility of a global definition similar to those in symplectic geometry and examine the implications of the Hodge star operator in this context.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- Some participants propose that the volume form can be expressed as dV = *1, where * is the Hodge star operator and 1 is the constant function.
- Others argue that this definition appears circular since the Hodge star is typically defined in terms of the volume form.
- There is a suggestion that the Hodge star operator can be defined locally using an oriented orthonormal basis without reference to the volume form.
- One participant mentions that defining the Hodge dual can be approached through different methods, including using a basis of p-forms and the metric's inner product.
- Concerns are raised about the relationship between alternating and symmetric powers, with some participants expressing uncertainty about their commutation properties.
- A proposed map from alternating powers of symmetric powers to symmetric powers of alternating powers is discussed, but doubts are expressed regarding its validity as an embedding.
- One participant reflects on their earlier misunderstanding regarding symmetries and anti-symmetries, indicating a shift in their perspective.
- Another participant acknowledges that previous comments may have been misleading and expresses gratitude for the contributions of others in the thread.
Areas of Agreement / Disagreement
Participants do not reach a consensus on the global definition of the volume form or the relationship between alternating and symmetric powers. Multiple competing views and uncertainties remain throughout the discussion.
Contextual Notes
Participants highlight limitations in their understanding of the definitions and relationships involved, particularly regarding the Hodge star operator and the properties of alternating and symmetric powers.