On Wednesday, February 12, 2025 at 12:08:13 PM UTC-7 Quentin Anciaux wrote:

AG, you're backpedaling again. You originally claimed that an infinite 
universe contradicts high temperature at the Big Bang, now you're just 
saying it's "possible" the universe was finite. Fine, but that’s not what’s 
debated—the issue is whether an infinite universe must be contradictory to 
high density, and it isn’t.


Please cease with accusations. I just see that stating a contradiction is 
too strong, and I believe it is possible that the high temperature implies 
very small volume.  You're relying on a metric which allows your pov, but 
that's just one metric. It doesn't prove that I am mistaken, or some 
experts who claim the size of the universe decreases as we go backward in 
time.. AG


The Cosmological Principle states that the universe is homogeneous and 
isotropic on large scales. 


And that it's the same everywhere. AG
 

This applies whether the universe is finite or infinite. Nothing about it 
requires the universe to be finite.


It does, if the universe's observable region is finite, then the entire 
universe is finite. AG
  

If the universe was spatially infinite at the Big Bang, it was just an 
infinite, uniformly dense, hot state. The fact that the observable universe 
shrinks as we go back in time doesn’t mean the entire universe had to be 
finite.


I am just claiming it could be finite, and that would explain its high 
temperature at or near the BB. The alternative is difficult to give 
credence to --- that it's infinite *and expanding*, and remains infinite as 
we go backward in time. AG 


If you’re now saying finiteness is just "possible" rather than required, 
then you’re conceding that your original contradiction doesn’t hold. So 
what’s left of your argument?


What's left is that you can't categorically rely on one metric to assert 
with finality what the physical reality might be. Apriori, hugely high 
early temperature is consistent with very small volume. AG 


Quentin 

Le mer. 12 févr. 2025, 20:04, Alan Grayson <[email protected]> a écrit :



On Wednesday, February 12, 2025 at 11:49:23 AM UTC-7 Quentin Anciaux wrote:

AG, your reasoning is flawed because it assumes a contradiction where none 
exists. An infinite universe doesn’t have to "become" infinite—it can be 
infinite at all times, just evolving in density and scale factor. High 
temperature and density at the Big Bang don’t require finiteness; they 
describe local conditions, not global topology.

Cosmological diagrams showing a "point" origin are simplifications based on 
the observable universe, not statements about the entire cosmos. The 
observable universe was smaller, but an infinite universe was never 
"shrinking" in the way you imply—just getting denser everywhere.


But this contradicts the Cosmological Principle (which might be wrong). AG 


You ask why it’s not even a possibility that finiteness is required for 
high density. The answer is that GR and the FLRW metric allow for infinite 
spatial extent at all times, even under extreme density conditions. There’s 
no physical principle preventing this, so the burden is on you to show why 
infinity at high density would be impossible.


Although I posed it as impossible, but that's probably going too far. I 
think It's possible that the entire universe is getting smaller as we go 
back in time, and this accounts for its super high temperature at or near 
the BB. AG 


Quentin 

Le mer. 12 févr. 2025, 19:41, Alan Grayson <[email protected]> a écrit :



On Wednesday, February 12, 2025 at 10:10:40 AM UTC-7 Quentin Anciaux wrote:



Le mer. 12 févr. 2025, 17:55, Alan Grayson <[email protected]> a écrit :



On Wednesday, February 12, 2025 at 2:09:58 AM UTC-7 Quentin Anciaux wrote:



Le mer. 12 févr. 2025, 09:55, Alan Grayson <[email protected]> a écrit :

If the age of the universe is finite, which is generally believed, then no 
matter how fast it expands, it can never become spatially infinite, So,* IF* 
it is spatially infinite, this must have been its initial condition at or 
around he time of the Big Bang (BB). But this contradicts the assumption 
that it was at a super high temperature at or around the time of the BB.


AG, your assumption that a finite-age universe must be spatially finite is 
flawed. If the universe is infinite now, it was infinite at the Big Bang,


That's what I wrote. AG 

just in a much hotter and denser state everywhere. The Big Bang wasn’t an 
explosion from a point 


I didn't assume that. What it actually is, or was, we don't know. But at 
that time it was hugely denser and hotter than at present. AG


No, you initially framed it as a contradiction—"If it’s infinite now, it 
must have been infinite at the Big Bang, but that contradicts the high 
temperature assumption." That’s what was wrong. There’s no contradiction 
between an infinite universe and high density. If you now accept that, 
great, but don’t pretend that was your original point.


I assumed that if the universe were infinite, it couldn't have become so in 
finite time, so IF infinite that must have been its initial condition. I 
later added, in summary, or that's what I meant to do, that this is 
contradictory to a super high temperature at the time of the BB. You claim 
this is inconsistent with GR. Can you prove that? AG


Yet, your reasoning implicitly relies on treating the universe as if it 
"shrinks" to a single location when run backward. A spatially infinite 
universe was never "smaller" in an absolute sense—just denser everywhere.


Well, that's what all the diagrams of the evolution of the universe show, 
that it becomes smaller as we go back in time, begins as a point, and what 
I've heard or read what some cosmologists claim. AG 

 

but a transition from an extremely dense, uniform state, which applies 
whether the universe is finite or infinite.

Eternal inflation suggests the universe was already infinite before the Hot 
Big Bang phase. 


Sure, provided eternal inflation is occurring, but it's speculative, as is 
my conclusion. Most cosmologists believe it was smaller in the past than at 
present, as implied by present day expanson run in reverse. AG 


No, they believe the observable universe was smaller. 


Why just the observable region? AG
 

That doesn’t mean the entire universe was ever finite.

 

The observable universe was once small and dense, but the entire universe 
could have been infinite at all times. 


Yes, COULD HAVE BEEN. I assumed, for the sake of argument, that it COULD 
NOT HAVE *BECOME* INFINITE IN FINITE TIME,  and THEN inferred what that 
implied; namely, that it became infinite at the time of the BB. Also, if 
you believe in the Cosmological Principle, if the observable universe was 
finite, then so was the entire universe.AG 

Spatial flatness doesn’t imply finiteness


I didn't assume it does. In fact, I assumed the reverse, as do 
cosmologists. I don't object to your criticisms, but you seem to be reading 
me with a jaundiced eye. AG

 

—flat, infinite universes expanding from a dense state are fully consistent 
with general relativity.

Does my conjecture conflict with GR, or is it also consistent? AG 


Yes, if you’re implying an infinite universe can’t be dense at early times 
or that it had to "become" infinite


I am assuming it couldn't become infinite in finite time, so, IF it is 
infinite now, it had to BE infinite at the time of the BB. AG 



There’s no contradiction between a spatially infinite universe and high 
density at early times. The problem isn’t with cosmology—it’s with your 
mistaken assumption that high density requires finiteness.


My assumption isn't necessarily mistaken. Rather, it's another possibility. 
AG 


No, it’s mistaken. Assuming high density requires finiteness is a 
misunderstanding of both GR and cosmology.


You claim it's not even a possibility. Why not? AG 


Quentin 


Quentin 

IOW, if we run the clock backward, the universe seems to get incredibly 
small, and for *this reason* incredibly hot, roughly analogous to a highly 
compressed gas. Therefore, it cannot have a flat global geometry, since 
such a geometry is infinite in spatial extent. QED. AG
 

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