tris_d said:
I think "curvatures" can not really exist in some 3D spatial volume as actual geometrical feature without reference frame against which it would be curved against. Actual curves would require actual reference frame and "empty space" contains nothing, so for it to contain some actual topology seem to be direct contradiction.
If you can explain some phenomena by supposing space is actually curved that I can not explain with the concept of potentials, gradients or fields, then I will submit space is actually curved as the best explanation.
This is a bit demanding. Let's take an example. Would you agree that the surface of the Earth is curved?
If you could come up with some combination of "fields and gradients and whatnot" to allow you to navigate on it successfully, would you suddenly declare that the Earth's surface was "not curved", and join the Flat Earth society?
I think it's probably rather more productive to focus on the math - which you didn't ask about, deciding to ask about the more phiilosohpihcal stuff first (which tends to lead to long, rambling, endless discssions ...
As far as the math goes, you'll need the concept of smooth curves connecting points. This may actually be the hardest part of the math, but it's easy enough to accept without getting into the precise defiitions of manifolds, topological spaces, and all that - especially if you're not too fussy.
You'll also need the concept of length, specifically the length of one of these curves.
Once you have those two down, that's really all you need to define curvature. You don't need "reference frames" and you don't need to worry about whether empty space is empty, half-empty, full, has polka-dots, or whatever. It's all irrelevant to what you do need.
Given this much, you can define a set of special curves, which are the shortest curves connecting two points in space. These are the geodesics (or rather a subset of them).
And you can follow in the steps of Einstein, and start to draw little quadrilaterals from these geodesics - and make them square, by making all four sides equal, and the diagonals equal as well.
Einstein's discussion of curvature is online at
http://www.bartleby.com/173/24.html
Then, when you compare the length of the diagonal to the length of the side of the square, you'll have your first indication of what "intrinsic curvature" is about. If you're on a plane, this ratio will be sqrt(t). If you're on a curved surface, like the Earth, you'll find that the length of the diagonals is not precisely the sqrt(2), but slightly different, getting further and further away from being sqrt(2) the larger you draw your figure.
The textbook mathematical treatment is perhaps a little more involved than this, but not really a whole lot. Generally in a textbook treatment one will at some point introduce the notion of parallel transport in fuller treatment. But you can think of parallel transport as the appication of a geometrical construction (Schild's ladder) based on "equal distances". So it's very helpful, and will eventually be needed, but you can get it from the notion of distances.
So to sum it all up - distances define geometry, and geometry defines curvature. That's really all there is to it.