- #106
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Well, I thought I would be straightened out within a couple of posts. I did not realize that
this is such a confusing topic.
I want to thank again everybody for their input and explanations.
I am still sorting some details out but I think that I now am starting to understand much better.
The key thing that I realized (and that Atyy emphasized) is that there is more than one definition
of diffeomorphism being used in the literature. Unfortunately, most people only use words in such discussions
and that leads to a lot of confusion when people use the same words to mean different things. Discussions
would be much clearer (and there would be much less arguing) if people would start by defining (mathematically!)
what they mean by a diffeomorphism (not only how the manifold is transformed but also how tensors are transformed), by general covariance, etc.
I think that Rovelli and Carroll are both very bright guys and I think that they understand what they
are talking about when they make statements about diffeomorphisms. They just have different definitions
of diffeomorphisms.
My understanding now is that according to a certain definition (adopted by Carroll among others),
invariance under diffeomorphisms is truly trivial and completely equivalent to invariance under a change
of coordinates. On the other hand, under Rovelli's definition of active diffeomorphisms, it is a non-trivial
statement to say that a theory is diffeomorphism invariant. GR is but QED, QCD, etc, are not.
As for general covariance, I think there are (at least) two ways to define that too.
In one definition, all theories can be made generally covariant and it does not tell us anything to
say that a theory is generally covariant. On the other hand, in understanding the resolution of the
hole argument, I have seen a definition of general covariance that is *not* trivial and that applies to GR
but not, say, to Newtonian gravity. And this is this definition that Rovelly has in mind in his book.
As for ''prior geometry", I am still not sure if this is used to refer simply to the fact that
spacetime intervals between points in spacetime are not defined a priori, i.e. that spacetime distances
are determined dynamically through Einstein's equations. Or if it is meant to also include what Rovelli
discusses in his book, which is the stronger (it seems to me) implication that not spacetime intervals
between points in spacetime are not defined independently of dynamics, but that the actual points in spacetime
have no physical signicance in the first place.
Anyway, these are just some thoughts. I am still trying to understand the details and I will surely come back with more
specific questions.
Thanks
this is such a confusing topic.
I want to thank again everybody for their input and explanations.
I am still sorting some details out but I think that I now am starting to understand much better.
The key thing that I realized (and that Atyy emphasized) is that there is more than one definition
of diffeomorphism being used in the literature. Unfortunately, most people only use words in such discussions
and that leads to a lot of confusion when people use the same words to mean different things. Discussions
would be much clearer (and there would be much less arguing) if people would start by defining (mathematically!)
what they mean by a diffeomorphism (not only how the manifold is transformed but also how tensors are transformed), by general covariance, etc.
I think that Rovelli and Carroll are both very bright guys and I think that they understand what they
are talking about when they make statements about diffeomorphisms. They just have different definitions
of diffeomorphisms.
My understanding now is that according to a certain definition (adopted by Carroll among others),
invariance under diffeomorphisms is truly trivial and completely equivalent to invariance under a change
of coordinates. On the other hand, under Rovelli's definition of active diffeomorphisms, it is a non-trivial
statement to say that a theory is diffeomorphism invariant. GR is but QED, QCD, etc, are not.
As for general covariance, I think there are (at least) two ways to define that too.
In one definition, all theories can be made generally covariant and it does not tell us anything to
say that a theory is generally covariant. On the other hand, in understanding the resolution of the
hole argument, I have seen a definition of general covariance that is *not* trivial and that applies to GR
but not, say, to Newtonian gravity. And this is this definition that Rovelly has in mind in his book.
As for ''prior geometry", I am still not sure if this is used to refer simply to the fact that
spacetime intervals between points in spacetime are not defined a priori, i.e. that spacetime distances
are determined dynamically through Einstein's equations. Or if it is meant to also include what Rovelli
discusses in his book, which is the stronger (it seems to me) implication that not spacetime intervals
between points in spacetime are not defined independently of dynamics, but that the actual points in spacetime
have no physical signicance in the first place.
Anyway, these are just some thoughts. I am still trying to understand the details and I will surely come back with more
specific questions.
Thanks