Garth said:
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If you ask why was the universe so compacted in the first place, the answer is all we do know is that if you trace back the expanding universe in time you inevitably tend towards a singularity called the Big Bang, with zero volume, infinite density and temperature, at which the known laws of physics break down. - And how!
I agree with lots of what you say---and how you lay out the various viewpoints---but i think this is incomplete.
If you trace back using quantized General Relativity (any of several different alternatives) you don't get to a singularity.
You continue tracing back though a moment of high (but not infinite) density and high (but not infinite) temperature and you keep on tracing back. As you trace back into the contracting phase, the density and the temperature get less. This takes care of the horizon problem, that Inflation Scenarios were invented to solve.
If you use 1915 General Relativity as your model, to trace back with, then you do get to a singularity. But this is not
inevitable because one is not forced to use 1915 Gen Rel. The fact that Gen Rel has singularities is widely believed to indicate that the theory is broken and people have been working for decades to fix the theory expecting that this would eliminate the singularities. It appears they now have a workable quantization, with a good classical limit, and that it has, as expected, fixed the "Big Bang" singularity. It is your choice how seriously to take the growing number of papers about this. I will get some references in case anyone wants to sample them.
What you get when you trace back in time depends on the model used to trace back with. it is no longer inevitable that one should use classical 1915 Gen Rel, so it is no longer inevitable that one gets to a singularity and has to stop tracing back.
A nice thing is that Loop cosmology has a good classical limit. It only disagrees for the first 10
-40 second of the expansion or so, after that it converges to classical or semiclassical behavior. So the quantized version only differs right around the big bang, which is where it needs to be different in order to eliminate the singularity and let you continue tracing back into the contraction phase.
Ashtekar and Bojowald have both discussed this convergence to the classical limit in various papers. there is, by now, a long list of papers by a lot of different researchers.
Your main point, Garth, is something else----physics is not about why/who.
I agree with that main point.
This business about the singularity is different. I contend that one does not inevitably encounter it.
If a person believes in Creator then there is no more reason for that Creator to have been around at the beginning of the observed expansion (at the socalled "Bang") than for Him to have been on hand in 1914 at the beginning of the First World War or for the first broadcast of "I Love Lucy". Theologically speaking, the classical ex-"Bang" is just another moment in history, as far as anyone knows.
The physics laws that apply to that moment should, as you indicated, be fascinating to discover, if we are even able to discover them! Certainly present laws do not cover those extreme conditions.
It is my feeling that the "Big Bang" should be scrubbed clean of any special theological interest so that one can study it dispassionately as one would anything else. More people are calling it the "Bounce" these days, which is probably more descriptive and less spiritually pornographic.