Fredrik
Graduate Poster
- Joined
- Jun 17, 2004
- Messages
- 1,912
It isn't possible to get a mental picture of it, for two reasons:I don't have a problem with "curvature"; that's a commonly understood word, and can generally be related to, but "space-time curvature", what does that look like?
a) Space-time is four-dimensional, and we can only picture three.
b) When we picture a curved two-dimensional surface, we always picture the curvature as a deformation into a third dimension, but the space-time manifold is curved without being deformed into a fifth dimension.
That's why you need differential geometry to define what curvature means.
This is one way of explaining a small part of it in plain English: Imagine transporting a tangent vector along a very short closed curve while trying to keep it pointing in the same direction. If the tangent vector isn't pointing in the same direction when you get back, and that effect persists when you shrink the loop to zero length, then the space-time manifold is curved at that location.
Unfortunately that doesn't explain what a manifold is, what a tangent vector is or what it means to keep a tangent vector "pointing the same way" and it doesn't tell us how large the curvature is. Differential geometry explains all of those things.
I guess you can say that it is. That "axiom" (or whatever we should call it) is what defines the theory. Everything else is derived from it. But this is how it is with any theory. The axioms define the theory, and you use them to derive everything else.I understand, but the theories of relativity, or our understanding of gravity, the way you explain it, seems like one entire axiom.
I could go into some detail about how the theory is used. For example, suppose we want to know what GR says about the behavior of matter in the universe on very large scales. First we note that on large scales matter is distributed very uniformly across the universe. So we decide to insert a completely uniform distribution of matter into the right-hand side of Einstein's equation, and see what comes out of the left-hand side. We find three solutions, all of them describing an expanding universe. All of them have a "big bang" singularity in the past. One of them says that space is finite and that the universe will end in a "big crunch". The other two say space is infinite and will expand forever.
That's usually how it's done. Decide what kind of matter distribution you're interested in, insert an idealized version of that into the right-hand side and see what comes out of the left-hand side. The result should be an approximate description of what you're interested in.
You could do it the other way too: Decide what kind of space-time geometry you'd like to study, insert it into the left-hand side, and see what kind of matter distribution comes out of the right-hand side. This is how you'd have to do it if you e.g. want to know what GR says about sci-fi stuff like time travel, wormholes and warp drives.
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