On 11/10/2017 4:06 AM, Alan Grayson wrote:


On Thu, Nov 9, 2017 at 10:32 PM, Brent Meeker <meeke...@verizon.net <mailto:meeke...@verizon.net>> wrote:



    On 11/9/2017 9:15 PM, Alan Grayson wrote:


    On Thu, Nov 9, 2017 at 10:05 PM, Brent Meeker
    <meeke...@verizon.net <mailto:meeke...@verizon.net>> wrote:



        On 11/9/2017 8:55 PM, agrayson2...@gmail.com
        <mailto:agrayson2...@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
            <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.

If it's flat or has negative curvature then the equations imply it's infinite or perhaps periodic (no matter what the scale factor is). If the curvature is positive then it's finite and closed and the scale factor can be taken to be the radius, so it indeed starts small in the absolute sense.  Atkatz and Pagels showed that only FRW universes that are closed (positive curvature) or De Sitter (flat with a positive cosmological constant) can "tunnel out of nothing".

http://www.quantum-gravitation.de/media/99f63994b9064eb6ffff8004fffffff2.pdf

So most cosmologists liked the closed universe model, until it was found that expansion is accelerating.  So now more of them look to some modification of the De Sitter space universe.

Brent

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