Liz,

In my theory one possible explanation of inflation could be an initial vast 
difference in the rates of p-time and clock time. I'm not saying that is 
the only explanation but it is a consistent one in my theory.

Thus it is meaningful to derive the radius of my proposed 4-dimensional 
hyperspherical universe to test that theory among others. If we compare the 
13.7 billion CLOCK time radius with some quite different P-time radius then 
we can begin to narrow that down and get some quantitative measure of the 
differences in rates.

Edgar



On Thursday, January 30, 2014 6:47:26 PM UTC-5, Liz R wrote:
>
> Omega=1 (to within 0.4%) which means the universe is very close to flat 
> (or even "hyperflat"). This is what would be predicted by inflation (which 
> is just as well, because I believe inflation was invented specifically to 
> solve the "flatness problem" !)
>
> If one treats the universe as having uniformly expanded from a point in 
> hyperspace, this measurement would make it very large (and hence, naively 
> one would think it was very old). But of course inflation means the 
> expansion was very, very nonuniform. Assuming the universe is a 
> hypersphere, it blew up to a huge size (by a scale factor of 10^78) in a 
> very short time (around 10^-33 sec), and then continued to coast at a much 
> reduced speed thereafter. This makes any measurement of the universe's 
> (hyper-) radius unlikely to give us a useful answer concerning "p-time" 
> (taken as roughly the distance of the universe from its hypothetical origin 
> in hyperspace divided by how fast it is expanding away from that point, I 
> assume).
>
> If this was a useful calculation, I think it would be reasonable to treat 
> the universe as an ideal fluid, where the only bound systems are atoms, for 
> the purpose of getting a rough answer. But I doubt that it would give any 
> sort of useful answer, assuming inflation really happened.
>  

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