WaveJumper said:
...the universe would still be a zero-dimensional "point"(aka Singularity), ...
What are your thoughts on this?
Singularity does not mean "point", it means the breakdown of a math model. We have no reason to suppose that singularities actually exist in nature.
You might get something out of reading "A Tale of Two Singularities" at Einstein-online. It is just a page. The E-o index is in my sig.
Quite a lot of current research in cosmology is with
non-singular models. These are math models that don't blow up and stop computing, as you work back in time. In other words people are interested in what really happened around the big bang, so they are attempting to develop models that are more realistic.
The classic 1915 theory had breakdowns of various shapes and sizes. Not all its singularities were zero dimensional points. That is another reason why it is a bad idea to equate singularity with point. Singularities exist in theoretical models, not in nature, and even in the context of a model, a singularity is not necessarily a point. There can be an extensive region of breakdown. A breakdown usually involves something that ought to be finite running off to infinity---the model stops computing sensible answers.
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One of the postulates of the Big Bang theory taken from GR says that the universe is not expanding into anything, but that it's the metric that's expanding.
That's right! And GR says space has no physical existence. It does not attribute objective reality to points, or spots, or locations whether in space or spacetime. You only get points when you fix on some definite artificial coordinate system.
In the most basic sense, to say that an observer, or a star, or a galaxy is
stationary, means that it is at rest with respect to the matter of the early universe---the source of the background radiation. It doesn't mean that the observer "stays at the same point" because there are no points. In artificial coordinate systems yes, but not in nature.
Points/locations are an artificial human invention and to define them you have to go thru a whole rigamarole of establishing a coordinate system, which in the end will probably involve anchoring to some material thing like a star or referring to the background radiation. We wave our arms but in the end our feet are still on the ground.
The idea of metric expansion says that two points in space remain at the same spots but the distance between them grows(while these two points remain at their same locations).
This doesn't make sense to me. What are points? What are spots? What are locations?
What does it mean to say that a point stays at the same point? Or that a spot stays at the same spot?
I like your mentioning metric expansion, but I imagine it differently. I picture two galaxies (or two observers) both of which are at rest relative to background. Their being at rest just means that neither is seeing a doppler hotspot in the background radiation. The distance between them is measured and found to be increasing.
What I'm trying to show here is a way to picture metric expansion in a completely
non-abstract way. It is supposed to be operational. Two real observers, they each look around and discover that the background is the same temperature in all directions, so they are both at rest. Then they proceed to measure the distance between them, which I agree is a technical problem, radar, synchronizing clocks etc. It isn't trivial, but somehow they manage to measure and keep track. Maybe other observers help. Anyway these two stationary observers discover the distance between them is increasing.
So far, nothing as abstract as a point, or a coordinate system, or spacetime, has been introduced into the story. You could do that though. You could introduce a system of socalled
comoving coordinates. They are technically useful as long as you stay within the range where they are applicable. Abstractions have limits to their applicability. Comoving coordinates break down if you go back too far. At least the ones I'm used to. With abstractions you have to know when to stop.
I think your post has a good idea, metric expansion, but it suffers from pushing an abstraction too far---to where the classic model develops a singularity.
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Now I'm going to contradict what I've said, and say that your post is right in a way. Some of the people who work on non-singular cosmology models actually do construct coordinate systems that don't break down! The metric bounces. There is a contraction which never goes singular (the density never blows up) and when the density reaches a very high level there's a bounce and expansion starts.
In those bounce models you really could have two mathematically defined points which would get closer and closer for a while, and then farther and farther apart. I have to admit that this looks very similar in some respects to what you were talking about.
So it looks like I'm hemming and hawing a lot on this one. Fence sitting. Maybe someone else will have a more definite reaction.