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stevendaryl said:Here is a way of thinking about theories that perhaps helps to clarify the sense in which GR is simpler than Newtonian gravity, in terms of covariance.
As people have pointed out, any theory of physics can be written in a covariant form. However, when one writes Newtonian physics in a covariant form, one finds that there is a "nondynamic" scalar field--Newton's universal time. It's nondynamic, in the sense that matter and energy and so forth don't affect it.
If you write Special Relativity in a covariant form, you will find that it has no nondynamic scalar fields. But it has a nondynamic tensor field, namely the metric tensor.
In General Relativity, there are no nondynamic scalar, vector or tensor fields. All the geometric fields are dynamic, they are affected by matter and energy.
I agree with this, and it is what the reference WNB gave in post#2 is formalizing (based on the approach given by Anderson in 1967 - where I first encountered it).
I realized there is a further terminological confusion going on, which I have contributed to (
). Within covariantly formulated theories, one may produce scalar invariants. However this sense of an invariant is different from formulating a principle of general invariance that is distinct from covariance. I have always preferred direct terminology like "no absolute objects" as the way way to formulate a theory filtering principle as opposed to a language for formulating any theory (general covariance) - rather than using the historically confused 'general invariance' for this. Some have used that the symmetry group of a theory ( as defined by Anderson - equivalently Straumann ) is the diffeomorphism group as the substantive (theory filtering) principle. To me, though, it all gets back to absolute objects, because absolute objects underpin this definition of the symmetry group of a theory.
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