phinds said:
Ok, first I want to say I'm ok with being wrong, but if I am I'll be very disappointed in Stephen Hawking because that will mean he said something that just plain isn't true (not just an oversimplification) and I can't see why.
Next, let's make sure we're addressing the right issue, because most of the "answers" there were to the wrong questions. Here's the three related questions:
1. What, in general, is a singularity? (a: a mathematical discontinuity, such as a divide by zero error)
2. What, specifically, is the nature of the Big Bang singularity? (My answer: r=0 @ t=0)
3. Do scientists believe the universe really started with a singularity? (a: no)
The question we're addressing here is #2 and if my answer is not correct, I'd like to know what the correct answer is. To be specific, I'd like to know what the relative diameter of the universe was at t=0 as implied by the equations...or, as I've seen it expressed, the average distance between galaxies or density.
Because I've seen over and over again it stated by sources that look credible that at the singularity, the universe's density and temperature would have been infinite. That's an awfully specific thing to be flat wrong and can't see what it could be an oversimplification of (that could be explained too...).
Yes, I agree that it approaches zero as a limit but it is my understanding that that is WHY we call it a singularity meaning a breakdown in the model, not a point in space.
If the quibble here is on the difference between being zero and approaching zero (with the density and temperature approaching infinity instead of being infinite), I think that would be an awfully petty quibble, since I think even most laypeople understand that "infinity" is not itself a number.
marcus said:
If Hawking gave you the impression that the Big Bang failure was only at a single point then he was being sloppy in his writing. He was writing for laypeople and couldn't be bothered to explain. We don't know for a fact that the U is spatial infinite but if it is, and we model it with GR in the usual way, then as you go back in time the theory fails across a broad front---you get meaningless results and infinities as you approach the start of expansion everywhere over a broad infinite extrent. With the classical (non quantum) theory the start of expansion completely fails to even be defined.
That's specific in the initial statement, but very non-specific with the explanation, so it doesn't satisfy my question. Specifically: what infinities do you get as you approach the start of the expansion? Density...? And does this answer apply to a finite universe?