On Sunday, August 25, 2019 at 12:21:37 AM UTC-6, Alan Grayson wrote:
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> On Saturday, August 24, 2019 at 10:16:56 AM UTC-6, Alan Grayson wrote:
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>> On Friday, August 23, 2019 at 11:32:47 PM UTC-6, Alan Grayson wrote:
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>>> On Friday, August 23, 2019 at 11:16:36 PM UTC-6, Alan Grayson wrote:
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>>>> On Friday, August 23, 2019 at 8:12:55 PM UTC-6, Lawrence Crowell wrote:
>>>>>
>>>>> On Friday, August 23, 2019 at 9:01:42 PM UTC-5, Alan Grayson wrote:
>>>>>>
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>>>>>> On Friday, August 23, 2019 at 7:48:19 PM UTC-6, Lawrence Crowell 
>>>>>> wrote:
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>>>>>>> On Friday, August 23, 2019 at 5:48:13 PM UTC-5, Alan Grayson wrote:
>>>>>>>>
>>>>>>>>
>>>>>>>>
>>>>>>>> On Friday, August 23, 2019 at 3:31:36 PM UTC-6, Lawrence Crowell 
>>>>>>>> wrote:
>>>>>>>>>
>>>>>>>>> On Thursday, August 22, 2019 at 12:37:40 AM UTC-5, Alan Grayson 
>>>>>>>>> wrote:
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>>>>>>>>>> On Wednesday, August 21, 2019 at 7:12:14 PM UTC-6, Alan Grayson 
>>>>>>>>>> wrote:
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>>>>>>>>>>>
>>>>>>>>>>>
>>>>>>>>>>> On Wednesday, August 21, 2019 at 3:13:11 PM UTC-6, Lawrence 
>>>>>>>>>>> Crowell wrote:
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>>>>>>>>>>>> On Tuesday, August 20, 2019 at 4:56:23 PM UTC-5, Alan Grayson 
>>>>>>>>>>>> wrote:
>>>>>>>>>>>>>
>>>>>>>>>>>>> https://en.wikipedia.org/wiki/Conformal_cyclic_cosmology
>>>>>>>>>>>>>
>>>>>>>>>>>>> Is this a viable theory for avoiding a BB interpreted as a 
>>>>>>>>>>>>> singularity? AG
>>>>>>>>>>>>>
>>>>>>>>>>>>
>>>>>>>>>>>> Penrose proposed a conformal identification of spatial infinity 
>>>>>>>>>>>> in the past and future i^±∞ of FLRW spacetimes. A cosmology 
>>>>>>>>>>>> expands and in 
>>>>>>>>>>>> the limit time → ∞ it transitions into a new cosmology. The de 
>>>>>>>>>>>> Sitter 
>>>>>>>>>>>> vacuum is not eternally stable, so the idea may have some germ of 
>>>>>>>>>>>> relevancy. I am not sure about how this would work with vacuum to 
>>>>>>>>>>>> vacuum 
>>>>>>>>>>>> transitions. The exponential expansion of the universe is a sort 
>>>>>>>>>>>> of time 
>>>>>>>>>>>> dependent conformal transformation with a small vacuum expectation 
>>>>>>>>>>>> for the 
>>>>>>>>>>>> scale field. To transition to a new cosmology, say with 
>>>>>>>>>>>> inflationary 
>>>>>>>>>>>> expansion, this means the vacuum expectation is increased.
>>>>>>>>>>>>
>>>>>>>>>>>> The overall physics community response to this has been tepid 
>>>>>>>>>>>> at best. There are some possible conflicts with observed data.
>>>>>>>>>>>>
>>>>>>>>>>>> LC
>>>>>>>>>>>>
>>>>>>>>>>>
>>>>>>>>>>> FWIW, ISTM that what GR might be indicating about the BB, is 
>>>>>>>>>>> that, insofar as it's a singularity, it couldn't have occurred, and 
>>>>>>>>>>> didn't 
>>>>>>>>>>> occur.  This is to say the universe didn't become infinitely small 
>>>>>>>>>>> in 
>>>>>>>>>>> spatial extent, like a mathematical point, but rather that there 
>>>>>>>>>>> was a 
>>>>>>>>>>> maximal finite value of its energy density, hugely high but not 
>>>>>>>>>>> infinite. 
>>>>>>>>>>> For this reason I find the cyclic models promising, although, as 
>>>>>>>>>>> you 
>>>>>>>>>>> rightly indicate, they're far from complete or bug-free. AG
>>>>>>>>>>>
>>>>>>>>>>
>>>>>>>>>> Which brings up a possibly relevant question: If the total energy 
>>>>>>>>>> of the universe occupied zero spatial volume (the presumed condition 
>>>>>>>>>> of the 
>>>>>>>>>> universe at t=o according to the BB theory), wouldn't that 
>>>>>>>>>> contradict the 
>>>>>>>>>> Uncertainty Principle? AG 
>>>>>>>>>>
>>>>>>>>>
>>>>>>>>> The total mass-energy content of the universe is zero.
>>>>>>>>>
>>>>>>>>> LC 
>>>>>>>>>
>>>>>>>>
>>>>>>>> Is that a provable fact, or something that can be measured? TIA, AG 
>>>>>>>>
>>>>>>>
>>>>>>> It is provable, because in general spacetimes there does not exist a 
>>>>>>> Gaussian surface to define mass. This sets the energy to zero. Think of 
>>>>>>> it 
>>>>>>> as meaning gravitational potential energy as negative is equal in 
>>>>>>> magnitude 
>>>>>>> to positive mass-energy. 
>>>>>>>
>>>>>>> LC
>>>>>>>
>>>>>>
>>>>>> If, using E=mc^2, one computes the rest energy of the material Earth, 
>>>>>> it seems implausible that this equals the negative potential energy of 
>>>>>> the 
>>>>>> Earth's gravitational field, to yield a net energy sum of zero. AG  
>>>>>>
>>>>>
>>>>> Consider the gravitation with expansion and cosmological constant. 
>>>>> This was first pointed out by Tolman many decades ago.
>>>>>
>>>>> LC 
>>>>>
>>>>
>>> Do you have links on this specific topic? TIA, AG 
>>>
>>>>
>>>> I will. But maybe in the meantime you could explain how, using E=mc^2 
>>>> and the negative potential energy of Earth's gravity field , you can get 
>>>> them to cancel out for an isolated Earth. Something very puzzling here. 
>>>> Additionally, ISTM that one would have an impossible task making a nuclear 
>>>> weapon from negative potential energy. What am I doing wrong, if anything? 
>>>> AG
>>>>
>>>
>> A test particle falling in a gravitational field gains in kinetic energy 
>> exactly what it loses in potential energy. However, what matters in this 
>> calculation is NOT the value of the potential energy at say two radial 
>> points in the falling path, say R2 and R1, but the DIFFERENCE in potential 
>> energy between these points. IOW, the potential energy is not well DEFINED 
>> as having some specific value. That is, one could add a constant to the 
>> potential energy at all points along the falling path and the calculation 
>> is unchanged. This is a long winded way of saying that it's a fallacy to 
>> add rest energy, calculated by mc^2, and gravitational potential energy, in 
>> an attempt to claim the total energy of the universe is exactly zero. Rest 
>> energy is well defined, but gravitational potential energy is not. AG
>>
>
> It's easy to calculate the (negative) potential energy (PE) of an OBJECT 
> in a gravitation field, but how does one calculate the PE of the field 
> itself?  I've looked on Internet but can't find an answer to this question, 
> upon which, it seems, the postulate of a zero energy universe rests. AG
>

Is the calculation done by simply integrating the energy density over all 
space containing the gravitational field? AG 

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