how can a universe that has expanded from a point explosion be anything other than a sphere, — T Clark
And while we're on the subject, how can portions of the universe which were next to each other 14 billion years ago be more than 14 billion light-years apart now? — T Clark
... which, in turn, suggests that something is missing. — jorndoe
Perhaps something an established unification of relativity and quantum mechanics could shed light on? — jorndoe
It was not from a point but a volume of points. Or rather a volume of points changed their scale. They always had a size (and an energy density) from the start. Then that size expanded (and cooled). — apokrisis
I like good yarns, just don't care calling them science with the purpose of creating some high ground. A good yarn is just that. We'll call this the volume of points yarn. Science always had a story to tell, whether or not it is worth telling. Was this within .4 uncertainty? — Rich
I l particularly ove the .4 uncertainty part of it. I suppose everyone is suppose to kowtow to this nonsense. That is how it is perpetuated. — Rich
I am unsure what you are suggesting though, Jorn, with the title and all... — TimeLine
how can portions of the universe which were next to each other 14 billion years ago be more than 14 billion light-years apart now? — T Clark
When we say "infinite" do we mean infinite volume or infinite mass? Both? Or something else? — T Clark
It seems that, by current findings, big bang inflation + expansion does not account for the spatial extent of the universe. — jorndoe
It seems that, by current findings, big bang inflation + expansion does not account for the spatial extent of the universe. Admittedly I haven't gone through the motions/calculations myself, but that was my thinking with the opening post. — jorndoe
how can a universe that has expanded from a point explosion be anything other than a sphere, — T Clark
It was not from a point but a volume of points. Or rather a volume of points changed their scale. They always had a size (and an energy density) from the start. Then that size expanded (and cooled). — apokrisis
You will have to explain why your comment makes any difference to my comment. — apokrisis
I asked what difference did your comment make. I did not say your comment was no different. — apokrisis
What we know for sure is that the Big Bang did not start from just a single of Planck-scale point right at the beginning. And indeed, something like inflation is needed to guarantee that the initial region that "banged" was already humongously large. — apokrisis
So the eternal and infinite version of inflation depends on an inflation event that spawns an unlimited number of big bangs. Ordinary inflation says our Big Bang suddenly took off and inflated a split second after it was first born. It wasn’t born inflating, but then inflation came along to make the universe sufficiently big and ensure that any local wrinkles were smoothed out and make the whole thing look as if it started off as perfectly flat and thermalised as possible. — apokrisis
I think you just want all the glory or something, hence why you are trying to answer questions directed to me. — TimeLine
Your shape and size of the universe is the observable universe of 46gly from earth and just to help ameliorate your understanding, the singularity - whilst it does not reference a single planck point - is a physically impossible point that we use to explain how the universe came to be. So the assumption is that the early conditions were infinitely dense at the size of 10^-28cm (with energies at 10^16 GeV) and that would mean that anything larger or smaller would blow the universe apart or suck it away — TimeLine
What? First of all, inflation is pushing omega to 1 and the asymptotic curvature would therefore be flattened by the expansion, thus the curvature would equal 0 or at least be very close to 0 and this would cause infinite expansion. The symmetry between these points is explained by fluctuations in the anisotropy of the cosmic microwave background and so the universe is isotropic and homogenous; the best way to explain thermal equilibrium (actually the only as far as I know) is inflation. — TimeLine
Who mention singularities? I didn’t. And what is the relevance of a length scale 100,000x the Planck length? I’m not following you at all. This is another series of irrelevancies. — apokrisis
Inflation doesn’t have to balance the kinetics of its expansion with its gravitational attraction. So an Omega balance is irrelevant. Inflation is about a scalar field that stays the same energy density while expanding exponentially. Repulsion dominates and gravity is simply impotent. — apokrisis
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