On Wed, Feb 5, 2014 at 7:38 PM, meekerdb <[email protected]> wrote:

>  On 2/5/2014 9:31 AM, Jesse Mazer wrote:
>
> --question 1 dealt with the question of how YOU would define p-time
> simultaneity in a cosmological model where there's no way to slice the 4D
> spacetime into a series of 3D surfaces such that the density of matter is
> perfectly uniform on each slice (and that uniform can be characterized by
> the parameter Omega), unlike in the simple FLRW model where matter is
> assumed to be distributed in this perfectly uniform way.
>
>
> I don't see that perfect uniformity is necessary.  We have calculated our
> epoch relative to the CMB as 13.8By.  I assume any other scientific species
> in the universe could do the same and so say whether they were 'at the same
> time' as measured by expansion of the cosmos.  I don't see how the
> existence of galaxies and galaxy clusters precludes this kind of
> measurement.
>


Using the CMB may give an approximate answer, but would you argue it could
distinguish between different simultaneity definitions that agree
approximately when averaged over large scales, but disagree somewhat about
the details of simultaneity in highly curved regions? For example, could
the CMB be used to define a unique definition of simultaneity in the
neighborhood of a black hole (where coordinate systems like Schwarzschild
coordinates and Eddington-Finkelstein coordinates and Kruskal-Szekeres
coordinates give very different definitions of simultaneity)? Edgar isn't
just claiming some approximate pragmatic truth about simultaneity, he's
claiming an absolute and exact truth about simultaneity in all
circumstances, I was asking if he thinks this truth can be empirically
determined to arbitrary precision even in principle, and if so what
empirical observations would be used.

Jesse



>
> Brent
>
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