On Friday, October 4, 2019 at 5:34:42 AM UTC-5, Alan Grayson wrote:
>
>
>
> On Friday, October 4, 2019 at 3:31:31 AM UTC-6, Lawrence Crowell wrote:
>>
>> On Thursday, October 3, 2019 at 8:13:22 PM UTC-5, Alan Grayson wrote:
>>>
>>> On Thursday, October 3, 2019 at 7:05:12 PM UTC-6, Lawrence Crowell wrote:
>>>>
>>>> On Thursday, October 3, 2019 at 8:01:49 PM UTC-5, Lawrence Crowell 
>>>> wrote:
>>>>>
>>>>> On Thursday, October 3, 2019 at 6:59:35 PM UTC-5, Bruce wrote:
>>>>>>
>>>>>> On Fri, Oct 4, 2019 at 9:54 AM Alan Grayson <[email protected]> 
>>>>>> wrote:
>>>>>>
>>>>>>>
>>>>>>> ISTM, that the argument the universe was NOT in thermo equilibrium 
>>>>>>> just before inflation is alleged to have begun, is extremely WEAK. 
>>>>>>> Thus, 
>>>>>>> it's illogical to claim that inflation "smooths out" the alleged NON 
>>>>>>> thermo 
>>>>>>> equiiibrium just before inflation begun. AG 
>>>>>>>
>>>>>>
>>>>>> That is essentially what I said. Lawrence is just replacing one set 
>>>>>> of unknown initial conditions with another, equally unjustified, set.
>>>>>>
>>>>>> Bruce
>>>>>>
>>>>>
>>>> In below & means δ. I forgot to replace them.
>>>>
>>>> LC
>>>>  
>>>>
>>>>>
>>>>> The entropy is S = A/4ℓ_p^2 +  quantum corrections, where these 
>>>>> corrections are ~ (&S/&h^a)k^a. Here h^a is tangent to the horizon and 
>>>>> k^a 
>>>>> is normal. This condition coincident on a null surface can appear on a 
>>>>> quantum extremal surface with null tangent g^s so that (&S/&h^a)k^a ≥ 
>>>>> (&S/&g^a)k^a by subadditivity. However, this surface occurs inside the 
>>>>> cosmological horizon. This means there is no equilibriium. Equilibrium is 
>>>>> only approximated by stretching the horizon out to enormous distance 
>>>>> after 
>>>>> the spatial surface has inflated. 
>>>>>
>>>>> It is the case that inflation does not tell us the whole story prior 
>>>>> to inflation. So one can say there are equally unknown initial 
>>>>> conditions. 
>>>>> However, the details of those are less important as the spatial manifold 
>>>>> is 
>>>>> stretched out. That means inflation does provide at least a working 
>>>>> system. 
>>>>>
>>>>> LC
>>>>>
>>>>
>>> Assuming the universe was incredibly tiny prior to inflation, and was 
>>> therefore causally connected, isn't it reasonable to assume that it had 
>>> reached thermo equilibrium *prior* to the onset of inflation? AG 
>>>
>>
>> Thermal equilibrium is not possible with quantum fields in curved 
>> spacetiome, nor is is likely in quantum gravity. The reason is not too hard 
>> to see. Suppose you have a black hole in a thermal background with the same 
>> temperature as its horizon T ~ 1/8M. The black hole has an equiprobability 
>> of absorbing or emitting a photon with energy δM The temperature then 
>> adjusts as T - δT ~ 1/8(M + δM) or T + δT ~ 1/8(M - δM) and is shifted away 
>> from thermal equality. This will then enhance the probability the black 
>> hole either then grows by absorbing more photons or by emitting them. There 
>> is no thermal equilibrium. Quantum gravitation is likely the same, for the 
>> effective specific heat of event horizons is negative. What I wrote above 
>> is in effect a more general form of this.
>>
>> Now a gemish of particles or a gas can be in thermal equilibrium in 
>> spacetime. 
>>
>
> *Doesn't this characterize the universe before inflation began? If not, 
> then what? AG*
>

No, the large plasma of particles was generated in the post inflationary 
period with reheating or the collapse of the vacuum or inflaton.

LC
 

>  
>
>> That was what was set up with inflation. The whole process of the early 
>> expanding universe is about there being episodes of approximate thermal 
>> equilibrium of particles, such as during the quark-gluon plasma phase, 
>> electroweak period, the QED equilibrium of electrons and photon or the 
>> plasma phase that ended by producing the CMB. 
>>
>> To think about physics one has to do a sort of Buddhist middle way. It is 
>> not good to either be too liberal or given to extreme speculations, but it 
>> is also not good to be overly conservative. 
>>
>> LC 
>>
>

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