- #141
jbergman
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- 175
These questions are somewhat subtle so I want to try and give my answer. First, I don't think that GR is a diffeomorphism invariant theory. Let ##R=(M,g)## and ##R'=(M', g')## then a diffeomorphism is just a smooth invertible map ##f: M \rightarrow M'##. It says nothing about the relationship between metrics. When you impose the additional condition on the pullback of the metric ##g=f^{*}g'##, you are describing an isometry. I think it's just an example of loose terminology in physics.PAllen said:I definitely agree it is more intuitive to approach kvf's starting from a congruence, which defines a vector field, and then require that any two points connected by a geodesic, when 'flowed' along the congruence by a fixed interval along congruence lines, results in a geodesic of the same length as before. Then showing that this property being true for any pair of points and any flow amount, is equivalent to more abstract definitions applied to the vector field itself. Note, of course, that none of this language involves coordinates (though building coordinates adapted to a killing flow ensures that certain features are present in the expression of the metric in those coordinates). Also note that none of this says anything about diffeomorphisms or coordinate changes.
However, I am quite confused by what any of this has to do with isometries. My understanding has been that for any diffeomorphism, when a pullback is applied to the metric, the result is an isometry. In particular, if you consider the coordinate transform from standard Minkowski coordinates to Milne coordinates, with the associated Milne metric, then for any pair of points connected by a geodesic in standard Minkowski coordinates, the result after transform, is still a geodesic of the same length when using the Milne metric.
See this discussion on https://physics.stackexchange.com/q...folds-physically-equivalent?noredirect=1&lq=1.
Now, in the case of space time there is really only one Universe (at least in this context), so conceptually we may want to restrict to maps to the same manifold ##f: M \rightarrow M## which leads to the auto-isometries which are isometries of a manifold to itself. In the case of the Milne coordinates we could define Minkowski space to be our pseudo-riemannian manifold, and just view the Milne coordinates as just one coordinate chart for that manifold. With the intrinsic definition of a manifold you have the manifold and then chart maps. This makes more sense for things like a sphere embedded in 3 space, but you can also have a 4-dimensional manifold, Minkowski space with alternative coordinate charts.
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