IIUC, the difference is huge. In the former case, the universe is open, spatially infinite with infinite mass (assuming a nonzero mass distribution on large scale everywhere), whereas the latter is closed, finite in spatial extent and mass. But I notice that most cosmologists claim the universe is *flat*, as in mathematically flat. Are they just speaking loosely and really mean the universe is ASYMPTOTICALLY flat? I find it contradictory for a universe which is finite in age, to be truly mathematically FLAT. TIA.
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Cosmologist think the universe is spatially flat. That just means triangles have interior angles summing to 180deg. It doesn't have anything to do with extent. But the universe is not flat in spacetime; it's expanding and at an increasing rate.
Brent
On 11/9/2017 3:10 PM, agrays...@gmail.com wrote:
IIUC, the difference is huge. In the former case, the universe is open, spatially infinite with infinite mass (assuming a nonzero mass distribution on large scale everywhere), whereas the latter is closed, finite in spatial extent and mass. But I notice that most cosmologists claim the universe is *flat*, as in mathematically flat. Are they just speaking loosely and really mean the universe is ASYMPTOTICALLY flat? I find it contradictory for a universe which is finite in age, to be truly mathematically FLAT. TIA.--
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The difference between spatially flat and asymptotically flat for a huge universe would be virtually impossible to distinguish by measuring the sum of angles in a triangle. Moreover, I don't see how spatially flat can have nothing to do with extent, since in applying Euclidean geometry we surely seem to be dealing with an infinitely extended plane. TIA.
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On Thu, Nov 9, 2017 at 4:42 PM, Brent Meeker <meek...@verizon.net> wrote:
Cosmologist think the universe is spatially flat. That just means triangles have interior angles summing to 180deg. It doesn't have anything to do with extent. But the universe is not flat in spacetime; it's expanding and at an increasing rate.
Brent
On 11/9/2017 3:10 PM, agrays...@gmail.com wrote:
IIUC, the difference is huge. In the former case, the universe is open, spatially infinite with infinite mass (assuming a nonzero mass distribution on large scale everywhere), whereas the latter is closed, finite in spatial extent and mass. But I notice that most cosmologists claim the universe is *flat*, as in mathematically flat. Are they just speaking loosely and really mean the universe is ASYMPTOTICALLY flat? I find it contradictory for a universe which is finite in age, to be truly mathematically FLAT. TIA.--
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On 11/9/2017 6:23 PM, Alan Grayson wrote:
The difference between spatially flat and asymptotically flat for a huge universe would be virtually impossible to distinguish by measuring the sum of angles in a triangle. Moreover, I don't see how spatially flat can have nothing to do with extent, since in applying Euclidean geometry we surely seem to be dealing with an infinitely extended plane. TIA.
Not necessarily. You could have periodic boundary conditions. But most cosmologists do assume the universe is infinite in spatial extent. Of course the flatness isn't measured by triangulation. It's measured by comparing the spatial spectrum of the CMB variations to model predictions with different mass densities.
https://arxiv.org/pdf/astro-ph/0004404
Brent
On Thu, Nov 9, 2017 at 4:42 PM, Brent Meeker <meek...@verizon.net> wrote:
Cosmologist think the universe is spatially flat. That just means triangles have interior angles summing to 180deg. It doesn't have anything to do with extent. But the universe is not flat in spacetime; it's expanding and at an increasing rate.
Brent
On 11/9/2017 3:10 PM, agrays...@gmail.com wrote:
IIUC, the difference is huge. In the former case, the universe is open, spatially infinite with infinite mass (assuming a nonzero mass distribution on large scale everywhere), whereas the latter is closed, finite in spatial extent and mass. But I notice that most cosmologists claim the universe is *flat*, as in mathematically flat. Are they just speaking loosely and really mean the universe is ASYMPTOTICALLY flat? I find it contradictory for a universe which is finite in age, to be truly mathematically FLAT. TIA.--
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On Thursday, November 9, 2017 at 8:00:45 PM UTC-7, Brent wrote:
On 11/9/2017 6:23 PM, Alan Grayson wrote:
The difference between spatially flat and asymptotically flat for a huge universe would be virtually impossible to distinguish by measuring the sum of angles in a triangle. Moreover, I don't see how spatially flat can have nothing to do with extent, since in applying Euclidean geometry we surely seem to be dealing with an infinitely extended plane. TIA.
Not necessarily. You could have periodic boundary conditions. But most cosmologists do assume the universe is infinite in spatial extent. Of course the flatness isn't measured by triangulation. It's measured by comparing the spatial spectrum of the CMB variations to model predictions with different mass densities.
https://arxiv.org/pdf/astro-ph/0004404
Brent
However flatness is measured, the criterion still seems Euclidean and hence infinite in extent if one believes the triangle measured has combined angles of 180 degrees. And I don't see how this is distinguishable from asymptotically flat for a huge but finite universe.
Moreover, it seems contradictory that a universe which has expanded for a finite duration, could be infinite in spatial extent. TIA.
On 11/9/2017 8:55 PM, agrays...@gmail.com wrote:
On Thursday, November 9, 2017 at 8:00:45 PM UTC-7, Brent wrote:
On 11/9/2017 6:23 PM, Alan Grayson wrote:
The difference between spatially flat and asymptotically flat for a huge universe would be virtually impossible to distinguish by measuring the sum of angles in a triangle. Moreover, I don't see how spatially flat can have nothing to do with extent, since in applying Euclidean geometry we surely seem to be dealing with an infinitely extended plane. TIA.
Not necessarily. You could have periodic boundary conditions. But most cosmologists do assume the universe is infinite in spatial extent. Of course the flatness isn't measured by triangulation. It's measured by comparing the spatial spectrum of the CMB variations to model predictions with different mass densities.
https://arxiv.org/pdf/astro-ph/0004404
Brent
However flatness is measured, the criterion still seems Euclidean and hence infinite in extent if one believes the triangle measured has combined angles of 180 degrees. And I don't see how this is distinguishable from asymptotically flat for a huge but finite universe.
It's not.
Moreover, it seems contradictory that a universe which has expanded for a finite duration, could be infinite in spatial extent. TIA.
It can if it starts off infinite. Remember the expansion in Einstein's equation is just a factor, not an absolute value.
Brent
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On Thu, Nov 9, 2017 at 10:05 PM, Brent Meeker <meek...@verizon.net> wrote:
On 11/9/2017 8:55 PM, agrays...@gmail.com wrote:
On Thursday, November 9, 2017 at 8:00:45 PM UTC-7, Brent wrote:
On 11/9/2017 6:23 PM, Alan Grayson wrote:
The difference between spatially flat and asymptotically flat for a huge universe would be virtually impossible to distinguish by measuring the sum of angles in a triangle. Moreover, I don't see how spatially flat can have nothing to do with extent, since in applying Euclidean geometry we surely seem to be dealing with an infinitely extended plane. TIA.
Not necessarily. You could have periodic boundary conditions. But most cosmologists do assume the universe is infinite in spatial extent. Of course the flatness isn't measured by triangulation. It's measured by comparing the spatial spectrum of the CMB variations to model predictions with different mass densities.
https://arxiv.org/pdf/astro-ph/0004404
Brent
However flatness is measured, the criterion still seems Euclidean and hence infinite in extent if one believes the triangle measured has combined angles of 180 degrees. And I don't see how this is distinguishable from asymptotically flat for a huge but finite universe.
It's not.
That's my point. No way of distinguishing flat from asymptotically flat for a huge universe, so the assumption of infinite spatial extent by cosmologists seems unwarranted. But as you note below, the universe could have begun with infinite spatial extent. But ours didn't AFAIK. It began as astronomically tiny and expanded via inflation.
On 11/9/2017 9:15 PM, Alan Grayson wrote:
On Thu, Nov 9, 2017 at 10:05 PM, Brent Meeker <meek...@verizon.net> wrote:
On 11/9/2017 8:55 PM, agrays...@gmail.com wrote:
On Thursday, November 9, 2017 at 8:00:45 PM UTC-7, Brent wrote:
On 11/9/2017 6:23 PM, Alan Grayson wrote:
The difference between spatially flat and asymptotically flat for a huge universe would be virtually impossible to distinguish by measuring the sum of angles in a triangle. Moreover, I don't see how spatially flat can have nothing to do with extent, since in applying Euclidean geometry we surely seem to be dealing with an infinitely extended plane. TIA.
Not necessarily. You could have periodic boundary conditions. But most cosmologists do assume the universe is infinite in spatial extent. Of course the flatness isn't measured by triangulation. It's measured by comparing the spatial spectrum of the CMB variations to model predictions with different mass densities.
https://arxiv.org/pdf/astro-ph/0004404
Brent
However flatness is measured, the criterion still seems Euclidean and hence infinite in extent if one believes the triangle measured has combined angles of 180 degrees. And I don't see how this is distinguishable from asymptotically flat for a huge but finite universe.
It's not.
That's my point. No way of distinguishing flat from asymptotically flat for a huge universe, so the assumption of infinite spatial extent by cosmologists seems unwarranted. But as you note below, the universe could have begun with infinite spatial extent. But ours didn't AFAIK. It began as astronomically tiny and expanded via inflation.
But you don't know that. According to Einstein's equations the visible part of the universe started at zero size. Of course no one takes that entirely seriously since at very small distances quantum mechanics must invalidate Einstein's equations.
Brent
Moreover, it seems contradictory that a universe which has expanded for a finite duration, could be infinite in spatial extent. TIA.
It can if it starts off infinite. Remember the expansion in Einstein's equation is just a factor, not an absolute value.
Brent
On Thu, Nov 9, 2017 at 10:32 PM, Brent Meeker <meek...@verizon.net> wrote:
On 11/9/2017 9:15 PM, Alan Grayson wrote:
On Thu, Nov 9, 2017 at 10:05 PM, Brent Meeker <meek...@verizon.net> wrote:
On 11/9/2017 8:55 PM, agrays...@gmail.com wrote:
On Thursday, November 9, 2017 at 8:00:45 PM UTC-7, Brent wrote:
On 11/9/2017 6:23 PM, Alan Grayson wrote:
The difference between spatially flat and asymptotically flat for a huge universe would be virtually impossible to distinguish by measuring the sum of angles in a triangle. Moreover, I don't see how spatially flat can have nothing to do with extent, since in applying Euclidean geometry we surely seem to be dealing with an infinitely extended plane. TIA.
Not necessarily. You could have periodic boundary conditions. But most cosmologists do assume the universe is infinite in spatial extent. Of course the flatness isn't measured by triangulation. It's measured by comparing the spatial spectrum of the CMB variations to model predictions with different mass densities.
https://arxiv.org/pdf/astro-ph/0004404
Brent
However flatness is measured, the criterion still seems Euclidean and hence infinite in extent if one believes the triangle measured has combined angles of 180 degrees. And I don't see how this is distinguishable from asymptotically flat for a huge but finite universe.
It's not.
That's my point. No way of distinguishing flat from asymptotically flat for a huge universe, so the assumption of infinite spatial extent by cosmologists seems unwarranted. But as you note below, the universe could have begun with infinite spatial extent. But ours didn't AFAIK. It began as astronomically tiny and expanded via inflation.
But you don't know that. According to Einstein's equations the visible part of the universe started at zero size. Of course no one takes that entirely seriously since at very small distances quantum mechanics must invalidate Einstein's equations.
Brent
If you're invoking QM, aren't you conceding it started out very small, if not exactly zero size? So it seems more plausible to assume it started out very small, surely not infinite. But according to your previous statements and those that I have read by cosmologists, the assumption of infinite spatial extent is generally accepted and IMO unwarranted.
Why is the closed universe model less favored when it was discovered that expansion is accelerating?
--TIA.
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I haven't read "Comprehensible Cosmos", but have done other reading. Vic had a way of glibly dismissing complex issues and it turned me off. Nevertheless, I basically respect his work. However, I really don't believe the Cosmos is Comprehensible. In fact, QM tells me the opposite. Ultimately, it's IRREDUCIBLY RANDOM as I think Bohr believed, and thus, IMO, INCOMPREHENSIBLE. God DOES play dice with the Universe. (Opinions can differ.)
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This is really a huge change in perspective (and FWIW, not one I am happy with).
I wonder; does the imposition of a positive CC ALSO automatically imply open, flat, and infinite? TIA, AG
I haven't read "Comprehensible Cosmos", but have done other reading. Vic had a way of glibly dismissing complex issues and it turned me off. Nevertheless, I basically respect his work. However, I really don't believe the Cosmos is Comprehensible. In fact, QM tells me the opposite. Ultimately, it's IRREDUCIBLY RANDOM as I think Bohr believed, and thus, IMO, INCOMPREHENSIBLE. God DOES play dice with the Universe. (Opinions can differ.)You seem to take for granted that Reality is the or a Physical Reality. But where that Physical reality comes from, and what is physical about it?Theoretical computer science, and its arithmetization, entails that if we assume the local finiteness of the observers, the observable correctly inferable of almost all finite observers emerges from a lattice of computations restrained by self-correctness self-referential relations.God get just asleep and lost itself innumerably in a labyrinth of dreams. technically, this should (and seems already) reduce the laws of the observable to arithmetical self-reference (unfortunately only well known by logicians (self-reference is handled in the arithmetical sense explained in Gödel 1931 paper.The Universal machine of Turing has a theology (a science of its own limitation toward truth if truth exists) which includes physics, so it is testable/refutable/improvable.All mystics said this: the Universe/Truth is in your head. So I suggest we compare the Universe which is in the head of the Universal (Turing) machine and what we infer from observations.You are right, there is something irreducibly random, if only the first person view of self-duplication i Arithmetic. But there are enumerable pieces of computations with an extreme redundancy in elementary Arithmetic (which is Turing complete). Physics is a first person plural view of arithmetic, and there must be derivation of the role of each pieces of its mathematics, like the group theory implied. Then the theology separates the true from the rationally justifiable, etc. The big discovery is the discovery of the universal machine (Emil Post, Alan Turing, Stephen Kleene, ...). It lives already in the diophantine polynomial equations.Bruno--
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Cosmologist think the universe is spatially flat. That just means triangles have interior angles summing to 180deg. It doesn't have anything to do with extent. But the universe is not flat in spacetime; it's expanding and at an increasing rate.
Brent
On Thursday, November 9, 2017 at 4:42:45 PM UTC-7, Brent wrote:Cosmologist think the universe is spatially flat. That just means triangles have interior angles summing to 180deg. It doesn't have anything to do with extent. But the universe is not flat in spacetime; it's expanding and at an increasing rate.
BrentI don't understand how a flat universe has nothing to do with extent.I don't understand the distinction; spatially flat (and therefore presumably infinite in extent?), but not flat in spacetime.Also, when it was discovered that the expansion is accelerating, did the solutions of the field equations which allowed tunneling from a vacuum and presumably automatically came with a positive CC (indicating expansion), also automatically come with a spatially flat (and presumably infinite in extent) geometry? Hard to grasp how a universe emerging from a vacuum could start out spatially flat and therefore IMO infinite in extent.TIA.