Discussion Overview
The discussion revolves around identifying a specific metric in which time is orthogonal to space, characterized by the condition that the time-space components of the metric tensor are zero everywhere. Participants explore the implications of this condition, its relation to known metrics, and the possibility of extending spatial slices throughout spacetime.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- One participant seeks to identify a metric where the time coordinate is normal to space, specifically where the time-space components of the metric tensor are zero.
- Another participant suggests the Minkowski metric but acknowledges it as a special case with restrictions on the spatial components.
- A participant clarifies that the desired metric has no restrictions on the spatial components and discusses the implications of having only certain derivatives constrained.
- There is a discussion about whether it is always possible to extend a spatial 3-space throughout spacetime under the given conditions, with one participant suggesting it may be possible based on the number of constrained derivatives.
- Contrarily, another participant argues that it is not always possible to find such a coordinate chart in every spacetime, providing Kerr spacetime as an example where the condition cannot be met.
- The term "hypersurface orthogonal" is mentioned, though it is noted that it typically applies to spacetimes with time translation symmetry, which does not encompass all cases of interest.
Areas of Agreement / Disagreement
Participants express differing views on the existence of a general term for the metric in question and whether it is possible to extend the spatial slices throughout spacetime. The discussion remains unresolved regarding the general applicability of the conditions described.
Contextual Notes
Participants note that the condition of having time normal to space may not hold universally across all spacetimes, and specific examples like Kerr spacetime illustrate the complexity of the issue. The discussion highlights the limitations of existing terminology and the need for further exploration of the topic.