On Sat, Feb 22, 2014 at 8:41 AM, Edgar L. Owen <edgaro...@att.net> wrote:

> John,
>
> Yes, that's my understanding, but that wasn't clear in your original post.
>
> However it is simply impossible for anything physical to be "literally
> infinite" when the nature of infinity as an unending PROCESS (forever add
> +1) rather than an actual number is understood.
>
> I hate it when otherwise intelligent physicists use infinite in the sense
> of just really really big!
>
> There simply are and can be no physical infinities. It's an impossible
> notion by its very definition.
>
> Edgar
>


Even worse Edgar when physicists substitute -1/12 for infinity.
Mathematica apparently rules our universe. Richard


>
> On Friday, February 21, 2014 2:16:48 PM UTC-5, John Clark wrote:
>>
>> On Fri, Feb 21, 2014 at 12:03 PM, Edgar L. Owen <edga...@att.net> wrot
>>
>> > I don't see how your CMB spot example works. Any 'spots' = features
>>> would not necessarily be caused by gravitation but could be caused by
>>> initial inhomogeneities as space itself expanded. Those are not necessarily
>>> ruled out. So I don't think your conclusion necessarily follows unless
>>> completely homogeneity is assumed, which it isn't in other theories such as
>>> brane traces and even enormously magnified = inflated quantum phenomena.
>>>
>>
>> No, complete homogeneity is not assumed. Quantum Mechanics says that an
>> unimaginably short time after the Big Bang the tiny cosmic fireball would
>> be very very homogenous but due to Heisenberg's Uncertainty Principle not
>> perfectly so, some parts of the fireball would be very slightly hotter and
>> denser than others. And the great thing about Quantum Mechanics is it
>> allows you to calculate numbers about all this, it can tell you just how
>> big the region would be and just how much denser and hotter it should be
>> and it can tell you how common variations from the norm will be. As the
>> universe expands these once tiny regions would enlarge too, and given
>> enough time gravity could make them grow too because slightly denser
>> regions would suck matter in from places that were slightly less dense so
>> with enough time there is no limit on how big they could get.
>>
>> But when we're looking at the CMBR we know how much variation to expect
>> from Heisenberg and we know that gravity had only 380,000 years to make
>> them bigger. And so we can figure out not just how large the biggest spots
>> should be but also how common spots of all sizes should be. And what we
>> predict the spectrum of spot sizes should be is exactly the same as what we
>> do in fact see. But we'd see something different if space were not flat,
>> the picture would be distorted and we'd see a different distribution of hot
>> and cold spots on the CMBR. But we see no such distortion so the Universe
>> at the largest scale must be flat, or at least nearly so, it's flat to at
>> least one part in 100,000 and could be absolutely flat.
>>
>> So regardless of how big our telescopes get at best the most of our
>> Universe we will ever observe is 0.0001% because 13.8 billion years is not
>> enough time for light from more distant parts of our universe to reach us.
>> And current observations are consistent with the universe being not merely
>> astronomically large but literally infinite.
>>
>>   John K Clark
>>
>>
>>
>>
>>
>>
>>
>>
>>  --
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