On 11/10/2017 10:01 PM, agrayson2...@gmail.com wrote:


On Friday, November 10, 2017 at 2:16:04 PM UTC-7, Brent wrote:



    On 11/10/2017 1:01 PM, agrays...@gmail.com <javascript:> wrote:


    On Friday, November 10, 2017 at 12:19:05 PM UTC-7, Brent wrote:



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


        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
                    <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
        
<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


    Modification of De Sitter will be flat and therefore open. I find
    the open universe model in contradiction to the finite age of the
    universe. Is this unreasonable?

    Well, if you have an infinite universe, and toward the past it is
    scaled by a factor a, and a->0 does the universes size go to zero?

    Why is the closed universe model less favored when it was
    discovered that expansion is accelerating?

    Because the De Sitter universe that can "tunnel from the vacuum"
    automatically has a positive cosmological constant.

    Brent


Unfortunately, my understanding of the scale factor and cosmological constant as they relate to the various geometries is insufficient to appreciate your comments. Maybe you could restate your above comments with that in mind. TIA.

Didn't you read Vic's "Comprehensible Cosmos"?  Why are you over here on the everythinglist asking physics questions anyway, Alan? You should try the stackechange or quora.

Brent

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