In the de Sitter cosmology the curvature of the spatial surface is 
determined by how it is embedded in the hyperboloid. Below is a diagram of 
such a hyperboloid of 2 dimensions where the spatial surface is the green 
curve. In this situation the spatial surface is infinite. If the spatial 
surface is embedded as a circle, such as the black circle around the 
coordinates q_1 and q_4, the spatial surface is a sphere S^3. Finally the 
hyperbolic spatial surface occurs if it is embedded along a more vertical 
direction. 

This is based on the idea the de Sitter manifold is embedded in 5 
dimensions with metric s = t^2 - u^2 - x^2 - y^2 - z^2, and the constraint 
s = 1 results in the dS metric. The metric reduced to 4 dimensions is

ds^2 = dt^2 - cosh(t√{3/Λ})dS^2

for dS^2 the spatial metric. The FLRW metric approximates this for large 
time with exp(t√{3/Λ}) ≈ cosh(t√{3/Λ}).

LC

[image: de Sitter space hyperboloid.png]




On Monday, January 20, 2020 at 8:55:06 AM UTC-6, John Clark wrote:
>
> I counted, the post I am now responding to had 10 iterated quotes, that's 
> quotes of quotes of quotes of quotes of quotes of quotes of quotes of 
> quotes of quotes. People are too lazy to trim anything and that's why in long 
> threads the signal to noise ratio declines exponentially and soon becomes 
> almost 
> unreadable. And that's why I'm starting a new one. 
>
> On Mon, Jan 20, 2020 at 7:49 AM Alan Grayson <[email protected] 
> <javascript:>> wrote:
>
> *> What I am established is that flatness is incompatible with a universe 
>> which had a beginning. So if it's flat, it never had a beginning; or else 
>> it did, and is closed, hyper-spherical in shape. AG*
>
>
> Are you talking about spatial curvature or spacetime curvature? By 
> "curvature" do you mean the angles of a triangle add up to something other 
> than 180 degrees, or do you mean if you keep going in one direction you 
> will eventually end up where you started? They are not necessarily the same 
> thing. 
>
> If the universe once expanded faster than the speed of light (as inflation 
> hypothesizes) then it's conceivable the angles of a triangle could add up 
> to be more than 180 degrees, so the universe would have a positive spatial 
> curvature like a sphere does, and yet you'd be going further and further 
> from your starting point into infinity and never return. And as long as 
> there had been a faster than light expansion at some point in the 
> universe's history if the angles of a triangle added up to less than 180 
> degrees then the universe would have negative spatial curvature, like the 
> shape of a saddle does, and you'd still never return to your starting place.
>
> John K Clark
>

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