On Monday, December 24, 2018 at 9:35:05 PM UTC, Bruce wrote:
>
> On Tue, Dec 25, 2018 at 4:43 AM John Clark <[email protected] 
> <javascript:>> wrote:
>
>> On Sun, Dec 23, 2018 at 5:38 PM Bruce Kellett <[email protected] 
>> <javascript:>> wrote:
>>
>> *> Flatness is explained if the unknown parameter k in the FRW solution 
>>> is set to zero. The the universe is always flat, no need to fine tune. 
>>> Setting k = 1 or k = -1 is just as fine-tuned or not as k=0.*
>>>
>>
>> There are an infinite number of ways space could have been curved but you 
>> picked one particular way (no curvature at all) for your initial conditions 
>> and did so for no particular reason other than to make the theory fit the 
>> facts that you already knew. Inflation explains why spacetime curvature 
>> could have any finite value whatsoever when the universe first came into 
>> existence and it would still look flat today even with our most sensitive 
>> instruments. It didn't have to start out with spacetime being zero or 
>> anything close to it, and that doesn't sound  fined-tuned to me.
>>
>> And the same thing is true of temperature, why are things at the same 
>> temperature when there was no time for them to come into thermal 
>> equilibrium? Inflation explains why, your explanation is they just did.  
>> Inflation says that  10^-35 seconds after the start of the universe and it 
>> had doubled in size about a hundred times  (and 10^35 seconds is a long 
>> long time compared to the Planck Time of 10^-43 seconds) the difference in 
>> temperature in our part of the universe would be almost zero but not 
>> precisely zero due to random quantum variations, and quantum theory allows 
>> you to calculate the intensity and size of what those temperature 
>> variations should have been. And you can also calculate what those 
>> temperature variations would evolve into after the universe has been 
>> expanding for 380,000 years, and what we calculate and what we see are the 
>> same.
>>
>> That's also how we know that at the very largest scale the universe is 
>> in general flat. They did this by looking at the oldest thing we can 
>> see, the Cosmic Microwave Background Radiation (CMBR) formed just 380,000 
>> years after the Big Bang. So if we look at a map of that background 
>> radiation the largest structure we could see on it would be 380,000 light 
>> years across, spots larger than that wouldn't have had enough time to form 
>> because nothing, not even gravity can move faster than light, a larger lump 
>> wouldn't even have enough time to know it was a lump. 
>>
>> So how large would an object 13.8 billion light years away appear to us 
>> if it's size was 380,000 light years across? The answer is one degree of 
>> arc, but ONLY if the universe is flat. If it's not flat and parallel lines 
>> converge or diverge then the image of the largest structures we can see in 
>> the CMBR could appear to be larger or smaller than one degree depending on 
>> how the image was distorted, and that would depend on if the universe is 
>> positively or negatively curved.  But we see no distortion at all, in this 
>> way the WMAP and Planck satellite proved that the universe is in general 
>> flat, or at least isn't curved much, over a distance of 13.8 billion light 
>> years if the universe curves at all it is less than one part in 100,000.
>>  
>>
>>> >> It would seem to me that if two theories can explain observations 
>>>> then the one with the simpler initial conditions is the superior. 
>>>>
>>>
>>> *> The trouble is that inflation is not  a simple theory. Where does the 
>>> inflation potential come from?*
>>>
>>
>> From the same place gravitational potential does I suppose, but inflation 
>> would be simpler, in General Relativity gravity needs a tensor field but 
>> inflation only needs a scalar field.
>>  
>>
>>>  > *Why don't we see the inflaton?*
>>>
>>
>> Maybe we do see it, maybe the acceleration of the universe we see today 
>> is the inflation field at work having undergone a  phase change when the 
>> universe was 10^-35 sec old and switched into a much lower gear. Or maybe 
>> not. Andrei Linde thinks the inflation field decayes away like radioactive 
>> half life, and after the decay the universe expanded at a much much more 
>> leisurely pace. But for that idea to work Guth's the inflation field had to 
>> expand faster than it decayed, Linde called it "Eternal Inflation". Linde 
>> showed that for every volume in which the inflation field decays away 2 
>> other volumes don't decay. So one universe becomes 3, the field decays in 
>> one universe but not in the other 2, then both of those two universes 
>> splits in 3 again and the inflation field decays away in two of them but 
>> doesn't decay in the other 4.  And it goes on like this forever creating a 
>> multiverse. 
>>
>> If any of this is true we may be able to prove it because Eternal 
>> Inflation would create gravitational waves with super long wavelengths that 
>> would produce very slight changes in the polarization of the cosmic 
>> microwave background radiation that we should be able to detect before 
>> long, assuming they exist.
>>
>
> You seem to be convinced by inflation theory. I am a lot more sceptical 
> because I see problems that you brush away contemptuously. Why has the 
> inflation not been seen at LHC? If it decayed into ordinary matter, it must 
> couple to ordinary matter, and so can be produced in high energy 
> collisions. But no evidence for any such particle has been found. Inflation 
> does not solve the horizon problem, either. At the end of the inflationary 
> period, the temperature was absolute zero everywhere -- no fluctuations. 
> The hot big bang came from the reheating phase where the inflation field 
> decayed into ordinary matter. As a quantum process, this would have 
> occurred randomly everywhere, so there would have been no uniformity in 
> temperate at all.
>

Do you have a typo at end? Did you intend to write "...  so there would 
have been no NON uniformity in temperature at all." AG


> Bruce 
>

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