On Wednesday, February 19, 2025 at 2:46:42 AM UTC-7 Quentin Anciaux wrote:
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. But if we're referring to a collapse not quite to zero volume, spacetime exists for a BH horizon to form. Also, if you grant that spacetime can contract or expand, are you not implicitly assuming a finite universe? AG 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. ISTM that they're essentially equivalent, that one implies the other and vice-versa. AG 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 -- You received this message because you are subscribed to the Google Groups "Everything List" group. To unsubscribe from this group and stop receiving emails from it, send an email to [email protected]. To view this discussion visit https://groups.google.com/d/msgid/everything-list/d533d2d5-c478-45c3-8a18-d2f17b23653bn%40googlegroups.com.
