On Sunday, October 6, 2019 at 6:04:22 PM UTC-6, Lawrence Crowell wrote:
>
> On Sunday, October 6, 2019 at 2:50:51 PM UTC-5, Alan Grayson wrote:
>>
>> On Saturday, October 5, 2019 at 1:27:49 PM UTC-6, Lawrence Crowell wrote:
>>>
>>> On Saturday, October 5, 2019 at 11:41:25 AM UTC-5, Alan Grayson wrote:
>>>>
>>>> On Saturday, October 5, 2019 at 7:57:59 AM UTC-6, Lawrence Crowell 
>>>> wrote:
>>>>>
>>>>>
>>>>>
>>>>> They came to equilibrium, and what thermal fluctuations that deviated 
>>>>> away from equilibrium were "ironed out" by inflation. 
>>>>>
>>>>
>>>> It's the "ironed out" that I don't understand. If there were some 
>>>> fluctuations, small deviations from thermal equilibrium, why would a 
>>>> sudden 
>>>> expansion attenuate them? It makes more sense to me that the universe was 
>>>> already very close to thermal equilibrium during inflation, and inflation 
>>>> *preserved* this state. BTW, I am not "belaboring" anything here; 
>>>> rather, I am trying to resolve, or possibly modify, a key element of the 
>>>> inflation model. AG
>>>>
>>>
>>> This is why these post with you drive me nuts. It is for the same reason 
>>> that if waves are stretched out they are made more IR. If clumps are 
>>> stretched out, think hard speed bump vs a soft one that is spread out, or 
>>> if curvatures are stretched these occur on a low energy or larger scale.
>>>
>>> LC
>>>
>>
>> Bruce has a dim view of inflation theory. He says it's a solution seeking 
>> a problem. He doesn't say, but if it's related to the present large scale 
>> homogeneity of the observable universe, it raises the issue of whether, 
>> just before or during inflation, the universe was already in thermal 
>> equiibrium. It's a reasonable question because, throughout that time, the 
>> universe was extraordinarily tiny and in causally connected. What's lacking 
>> in your reply, and possibly in the theory supporting inflation ON THIS 
>> PARTICULAR ISSUE, is a rigorous definition of thermal equilibrium, and 
>> whether the time scale of inflation (its duration), the size of the 
>> universe during that time, and the SoL, whether thermal equilibrium is 
>> definitely ruled OUT. Maybe it deviated by just one part in 100,000 and 
>> this is what is measured in the CMBR. If the question drives you nuts, it's 
>> probably because, to some extent, you share the world-view of the ruling 
>> elite in ancient Greece who found the questions of Socrates intolerable and 
>> insisted he drink the hemlock. My method is to test the claims of theories, 
>> and the more polemic the answers, the less confidence I have in their truth 
>> value.  That said, I thank you for the plausible information that particles 
>> became manifest with the decay of the original vacuum. AG
>>
>
> These questions by you drive me crazy because they go around and around. 
>

It's your problem, not mine; sort of an intolerance for detailed dialogue 
on deep and confusing issues. AG 

>
> Bruce is very conservative, too conservative I think. Inflation makes some 
> sense out of things, and while it is not a fundamental theory, it does push 
> ignorance back. It also has some measure of observational support. 
>

I agree with inflation wrt the flatness problem. Not sure exactly which 
part of inflation Bruce finds questionable. AG 

>
> LC
>

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