2014-02-06 Jesse Mazer <[email protected]>:

>
>
> On Thu, Feb 6, 2014 at 9:01 AM, Edgar L. Owen <[email protected]> wrote:
>
>> But recall that p-time is not a directly measurable quantity so
>> "arbitrary precision" does not apply. You still haven't grasped the concept
>> correctly. P-time has no direct measure, because the present moment is that
>> in which all measures, including those of clock time, are computed.
>>
>
> I don't recall you ever spelling that out in conversation with me, thanks
> for clarifying. In the past people had asked you about how to determine
> p-time and you had said things like "we should be able to compute p-time
> from Omega, the curvature of the universe" (in the post at
> http://www.mail-archive.com/[email protected]/msg47450.html). 
> So if you now say that determining which events are simultaneous in
> p-time is fundamentally impossible for any being within the universe, that
> answers what I was wondering about in question #1.
>

If that's the case... what good is it to entertain such "p-time"... it's
useless. Predict nothing, cannot be measured. What is p-time supposed to
solve ?


>
> Jesse
>
>
>
>>
>> Nevertheless the fact of existence of all observers and thus of
>> everything in the present moment is a direct empirical observation. Just
>> like consciousness it is not subject to measure, but that doesn't mean it
>> doesn't exist.
>>
>> Edgar
>>
>> On Thursday, February 6, 2014 12:47:05 AM UTC-5, jessem wrote:
>>>
>>>
>>>
>>> On Wed, Feb 5, 2014 at 7:38 PM, meekerdb <[email protected]> wrote:
>>>
>>>>  On 2/5/2014 9:31 AM, Jesse Mazer wrote:
>>>>
>>>> --question 1 dealt with the question of how YOU would define p-time
>>>> simultaneity in a cosmological model where there's no way to slice the 4D
>>>> spacetime into a series of 3D surfaces such that the density of matter is
>>>> perfectly uniform on each slice (and that uniform can be characterized by
>>>> the parameter Omega), unlike in the simple FLRW model where matter is
>>>> assumed to be distributed in this perfectly uniform way.
>>>>
>>>>
>>>> I don't see that perfect uniformity is necessary.  We have calculated
>>>> our epoch relative to the CMB as 13.8By.  I assume any other scientific
>>>> species in the universe could do the same and so say whether they were 'at
>>>> the same time' as measured by expansion of the cosmos.  I don't see how the
>>>> existence of galaxies and galaxy clusters precludes this kind of
>>>> measurement.
>>>>
>>>
>>>
>>> Using the CMB may give an approximate answer, but would you argue it
>>> could distinguish between different simultaneity definitions that agree
>>> approximately when averaged over large scales, but disagree somewhat about
>>> the details of simultaneity in highly curved regions? For example, could
>>> the CMB be used to define a unique definition of simultaneity in the
>>> neighborhood of a black hole (where coordinate systems like Schwarzschild
>>> coordinates and Eddington-Finkelstein coordinates and Kruskal-Szekeres
>>> coordinates give very different definitions of simultaneity)? Edgar isn't
>>> just claiming some approximate pragmatic truth about simultaneity, he's
>>> claiming an absolute and exact truth about simultaneity in all
>>> circumstances, I was asking if he thinks this truth can be empirically
>>> determined to arbitrary precision even in principle, and if so what
>>> empirical observations would be used.
>>>
>>> Jesse
>>>
>>>
>>>
>>>>
>>>> Brent
>>>>
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-- 
All those moments will be lost in time, like tears in rain. (Roy
Batty/Rutger Hauer)

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