On Tuesday, January 1, 2019 at 6:24:03 PM UTC, John Clark wrote:
>
> On Tue, Jan 1, 2019 at 3:41 AM <[email protected] <javascript:>> wrote:
>  
>
>> *> not all points external to an observer are receding at speed faster 
>> than light. Still, ISTM that inflation just preserves the temperature 
>> distribution which exists when it began,*
>
>
> The idea is before inflation a small volume was able to achieve thermal 
> equilibrium within itself even though the universe was very very young 
> because the volume was so small. But then that small volume started to 
> expand faster than light and exponentially doubled in size at least 100 
> times every 10^-35 seconds, and today that super tiny volume is our entire 
> observable universe. The FTL expansion is why very distant parts of the 
> CMBR are at almost exactly the same temperature even though today they are 
> not causally connected. 
>


But earlier you wrote that without inflation, the temperature anomalies 
would have been washed out anyway. 

Clark > If inflation didn't happen then after 380,000 years those spots of 
slightly higher and lower temperature would no longer exist because they 
would have been washed out by their surroundings ... .

So without inflation, the CMBR would have *more* uniformity in temperature 
than what it was initially. That's why I stated that inflation preserved 
the initial imperfect uniformity in temperature, but wasn't the *cause* of 
the uniformity. AG

And the random quantum variations that must have existed in that very tiny 
> volume before inflation started explains why the temperature of the CMBR is 
> *almost* the same everywhere but not exactly so.  
>
>  John K Clark 
>
>
>

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