Le ven. 21 févr. 2025, 09:58, Alan Grayson <[email protected]> a
écrit :

>
>
> On Friday, February 21, 2025 at 1:24:18 AM UTC-7 Quentin Anciaux wrote:
>
> Try to use the internet sometimes....
>
>
> https://www.astro.rug.nl/~weygaert/tim1publication/cosmo2019/cosmology2019.lect3a.cosmological_principle.pdf
>
> https://pages.uoregon.edu/jschombe/cosmo/lectures/lec05.html
>
>
> Interesting. TY.The Gamma Ray Bursts are pretty convincing to establish
> isotropy and homogeneity. One other thing. In Penrose's oscillating
> universe model, does he assume the volume expands and contracts
> periodically, or does he assume it remains infinite in volume throughout,
> and that the average distances between galaxies increases and decreases
> periodically? AG
>

It assumes it is infinite and remains infinite, only density varies.

Quentin


> Le ven. 21 févr. 2025, 09:11, Alan Grayson <[email protected]> a écrit :
>
>
>
> On Thursday, February 20, 2025 at 8:51:53 PM UTC-7 Alan Grayson wrote:
>
> On Thursday, February 20, 2025 at 2:45:02 AM UTC-7 Quentin Anciaux wrote:
>
> AG, while filaments and voids extend across hundreds of megaparsecs,
> isotropy only breaks down locally, not globally. If you look at one
> specific region, it may appear anisotropic, but if you average over
> sufficiently large volumes, the universe still appears statistically
> homogeneous and isotropic. Observations of the cosmic microwave background
> (CMB) and large-scale galaxy surveys confirm this—on scales larger than 1
> gigaparsec, the universe still obeys the Cosmological Principle.
>
>
> Can you cite a paper which supports your claim? Deep space surveys which
> show the filaments and voids at distances greater than hundreds of
> megaparsecs. So, since seeing is believing, at huge distances the CP seems
> to fail. Despite my skepticism, I am willing to read any paper that
> substantiates your claim. AG
>
>
> To observe filaments and voids, how far out are they to be viewed? If you
> go out 500 megaparsecs, that's slightly less than 1.6 billion light years,
> a small fraction of the radius of the visable universe, which 46 billion
> light years. At that distance, if they can be viewed, the universe doesn't
> seem to be isotropic. AG
>
>
> Regarding the universe emerging from nothing, if it were spatially
> infinite now, then yes—it would have had to be spatially infinite from the
> very beginning. An infinite universe doesn’t "grow" from a finite state in
> a finite time. If you assume the universe truly began from absolute
> nothing, then it must have instantaneously been infinite—which itself
> raises deep questions about the nature of such a transition. This is one of
> the reasons why many models (such as eternal inflation or cyclic universes)
> propose pre-existing states rather than a true emergence from nothing,
> which in itself is something miraculous.
>
>
> Every thing about the universe is miraculus if you think about it more
> deeply. I tried to form a model of the early universe which is simplest,
> and a finite bubble, arising from an infinite substratum, approximately
> spherical in shape, at an ultra-high temperature, seems to fill the bill.
> AG
>
>
> Quentin
>
> Le jeu. 20 févr. 2025, 10:14, Alan Grayson <[email protected]> a écrit :
>
>
>
> On Thursday, February 20, 2025 at 1:56:36 AM UTC-7 Quentin Anciaux wrote:
>
> AG, the Cosmological Principle (CP) applies at large scales, not at the
> scale of individual galaxies, filaments, or voids. While structure
> formation creates density variations, these variations average out when
> viewed over hundreds of megaparsecs. The CMB provides the earliest direct
> evidence of large-scale homogeneity, and while gravitational evolution has
> produced filaments and voids, the CP still holds statistically when
> considering the universe at a sufficiently large scale. The fact that
> structure forms doesn’t contradict the CP—it’s an expected consequence of
> small initial fluctuations growing under gravity.
>
>
> *When we can observe filaments and voids, aren't we observing way beyond
> hundreds of megaparsecs, and isotropy clearly breaks down? AG *
>
>
> Regarding the age of the universe, yes, it’s finite (around 13.8 billion
> years). If the universe is infinite now, then it must have been infinite
> from the beginning—infinity doesn’t "grow" in a finite time. This is why an
> infinite universe was already infinite at the Big Bang, just in an
> extremely dense and hot state. That’s not an opinion; it follows directly
> from how GR and the FLRW metric describe an infinite expanding spacetime.
>
> As for the Big Bang (BB), it is best understood as a transition rather
> than a singular "event." The BB represents the point where classical GR
> models break down, and physics needs quantum gravity to describe what came
> "before" (if that question even makes sense). The universe didn’t
> necessarily emerge from nothing—
>
>
> *Right, not necessarily, but if it did emerge from Nothing, could it have
> become infinite instantaneously? AG*
>
>
> the BB marks the beginning of our current phase of expansion, but there
> could have been a prior state (eternal inflation, a bouncing universe, or
> some other pre-BB phase). GR alone doesn’t tell us whether the universe
> "came into existence" at T=0—it just describes its evolution from an
> extremely hot, dense state forward. Look for hot big bang.
>
> Quentin
>
> Le jeu. 20 févr. 2025, 09:42, Alan Grayson <[email protected]> a écrit :
>
>
>
> 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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