Discussion Overview
The discussion centers on the concept of the "expansion of the universe," particularly focusing on the coordinate independence of cosmological redshift and the validity of the expansion tensor in general relativity. Participants explore theoretical implications, mathematical definitions, and the relevance of different observer perspectives.
Discussion Character
- Debate/contested
- Technical explanation
- Mathematical reasoning
Main Points Raised
- Some participants assert that the universe's expansion can be described in a coordinate independent manner, referencing the comoving congruence and the expansion tensor.
- Others challenge the validity of the expansion tensor, arguing it is misleading to use it as an argument for coordinate independence.
- A participant explains that cosmological redshift is an observable quantity that is inherently coordinate independent, detailing the process involving a photon's 4-momentum and its interaction with a comoving observer.
- There are claims regarding the mathematical definitions of tensors and pseudotensors, with some participants emphasizing the need for clarity in definitions across different contexts.
- Questions arise about the treatment of non-comoving observers and how the expansion tensor applies to them, with some arguing that there are no restrictions on the congruences used by different observers.
Areas of Agreement / Disagreement
Participants express differing views on the validity and implications of the expansion tensor, with no consensus reached on its role in demonstrating coordinate independence or its applicability to non-comoving observers.
Contextual Notes
Participants note limitations in definitions and the potential for varying interpretations of terms like tensor and pseudotensor, which may affect the clarity of arguments presented.