A black hole forms when mass collapses within an external spacetime,
creating an event horizon. The early universe wasn’t a localized collapse
within surrounding space—it was the entire spacetime itself contracting or
expanding. That’s why an event horizon doesn’t form around it.

The difference between homogeneous and isotropic is simple: homogeneity
means the universe has the same properties everywhere on large scales,
while isotropy means it looks the same in all directions. Together, they
describe a universe that doesn’t have a preferred center or edge, unlike a
collapsing object forming a black hole.

Quentin

Le mer. 19 févr. 2025, 10:20, Alan Grayson <[email protected]> a
écrit :

>
>
> On Wednesday, February 19, 2025 at 1:40:13 AM UTC-7 Quentin Anciaux wrote:
>
> AG, the key issue is that the universe isn’t collapsing into a localized
> region—it’s expanding/collapsing everywhere.
>
>
> I am not being sarcastic to ask if that's a fact based on solid physics or
> your opinion? AG
>
>
> A black hole forms when mass collapses within a surrounding spacetime,
> creating an event horizon. The early universe, however, was homogeneous and
> isotropic on large scales, meaning there was no "outside" region for an
> event horizon to form around it.
>
>
> Firstly, I have a hard time distinguishing between homogeneous and
> isotropic. Also, if we assume the volume shrinks close to, but not equal to
> zero, there would be a region where an event horizon could form. AG
>
>
> In GR, a universe that contracts to extremely high density doesn’t
> necessarily become a black hole—
>
>
> "Doesn't necessarily", but is it possible or absolutely precluded?  AG
>
> it follows different equations that describe a hot, dense state rather
> than a localized collapse. The FLRW metric describes a global evolution of
> spacetime, not a local gravitational collapse like a black hole. That’s why
> the early universe could be dense without forming a black hole—it didn’t
> have a surrounding spacetime to collapse into.
>
>
> As I posted earlier on another thread, there could be other metrics that
> predict a BH result close to the BB. AG
>
>
> Quentin
>
> Le mer. 19 févr. 2025, 09:33, Alan Grayson <[email protected]> a écrit :
>
>
>
> On Tuesday, February 18, 2025 at 11:19:45 PM UTC-7 Alan Grayson wrote:
>
> On Monday, February 17, 2025 at 11:59:45 PM UTC-7 Alan Grayson wrote:
>
> [image: Alan Grayson's profile photo]
> Alan Grayson
> 11:56 PM (1 minute ago)
> 
> 
> 
> to Everything List
> Running the clock backward, and assuming the physical size of the universe
> converges to a singularity with zero volume at T=0, will it form a Black
> Hole? TY, AG
>
>
> Let me pose the problem differently; if the entire *universe* contracted
> to almost zero volume, is there anything we know that would prevent it from
> becoming a BH? AG
>
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