On Thursday, February 20, 2025 at 12:22:32 AM UTC-7 Quentin Anciaux wrote:



Le jeu. 20 févr. 2025, 08:05, Alan Grayson <[email protected]> a écrit :



On Wednesday, February 19, 2025 at 11:54:52 PM UTC-7 Quentin Anciaux wrote:

AG, a Big Crunch scenario does not necessarily assume a finite universe. An 
infinite universe can also undergo a global contraction—meaning that while 
distances between galaxies shrink, the universe itself remains infinite at 
all times. A finite universe collapsing to zero volume in finite time is 
just one possibility, but it’s not required for a Big Crunch model. The 
idea of a finite universe is, of course, not beyond the pale—it remains an 
open question in cosmology.

Regarding infinite space and "unchanging volume," the key issue is that 
volume in an infinite universe is not a meaningful quantity in the way you 
are describing it. Yes, if the universe is infinite now, it was always 
infinite, but that doesn’t mean nothing changes—the scale factor determines 
how distances evolve. The phrase "volume cannot change" is misleading 
because in an infinite universe, there is no finite, well-defined total 
volume to begin with. Instead, we talk about the expansion or contraction 
of distances within that infinite space, which is physically meaningful.

Quentin


*Do you concede that the universe isn't isotropic or homogeneous? What is 
the nature of the singularity in the Big Crunch for a finite and infinite 
universe? How does it differ from the standard BH? AG *


AG, on small scales, the universe is neither isotropic nor homogeneous due 
to the presence of galaxies, filaments, and voids. However, on large 
scales, it is effectively homogeneous and isotropic, as confirmed by the 
cosmic microwave background (CMB) and large-scale surveys. The Cosmological 
Principle—which assumes large-scale homogeneity and isotropy—remains valid 
for describing the universe at scales beyond a few hundred megaparsecs.


*While the CMB is approximately uniform in temperature, but that's at 
380,000 years after the BB, but when we observe it at later times, there 
are huge filaments with a plethora of galaxies, separated by huge voids. 
This cannot be isotropic since the scale is hugely large. It's also not 
homogeneous if we consider the property of density. So, IMO, whereas the 
universe seems to satisfy the CP at 380,000 years, its subsequent evolution 
contradicts the CP. AG*

*Do you agree that the age of the universe is finite, so if it's infinite, 
that condition could not have evolved over its finite lifetime, but must 
have been its property as an initial condition? AG*


Regarding the Big Crunch singularity, it differs depending on whether the 
universe is finite or infinite:

Finite Universe: If the universe is closed and finite, a Big Crunch would 
resemble the time-reversed version of the Big Bang—space collapses to a 
singularity where density, temperature, and curvature diverge. It’s a true 
spacetime singularity in GR, where classical physics breaks down.


*Do you believe in the BB as a specific event, at time defined as T=0, from 
which the universe emerged from some underlying substratum? IOW, do you 
believe the universe came into existence at the BB? AG* 


Infinite Universe: If an infinite universe undergoes a Big Crunch, 
distances still shrink everywhere, but it remains infinite at all times. 
The singularity would be a global state of infinite density everywhere 
rather than a localized point. Unlike a black hole, this singularity isn’t 
"contained" within an event horizon—it involves the entire universe.

A black hole singularity, in contrast, is localized—it forms due to 
asymmetric collapse, creating an event horizon around a specific region of 
space. In a Big Crunch, there’s no such horizon enclosing the universe 
because space itself is collapsing uniformly (on large scales). That’s the 
fundamental difference: a black hole singularity is localized within 
spacetime, while a Big Crunch singularity is the entire spacetime itself 
collapsing.

Quentin 

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