On Saturday, February 8, 2014 5:19:12 AM UTC, Liz R wrote:
>
> I'm not sure you can distinguish a "unit of energy". These can be changed 
> from one for to another. Suppose an atom with an "age" (since it emerged 
> from the big bang) of 12Gy absorbs a photon with an "age" of 10Gy (although 
> a CMBR photon would presumably have an age of 400,000 years since no time 
> elapses for photons!) ... what's the age of the excited atom that results?
>
 
I suppose the most consistent way to answer that from the perspective I'm 
throwing out, would be to ask whether that clearly legitimate question is 
at a level of complexity we can reasonable hope to address, before having 
first finding a way to set things up at a much more generic level. It's at 
least arguable it isn't a reasonable expectation, the same way it wouldn't 
have been reasonable to solve so precisely for the generic principles in 
play by considering a car-crash with no basic theoretical framework for 
isolated laws to begin with. By 'basic' I obviously mean in a totally 
gratuitous extreme of the generic as already indicated!  

>
>
> On 8 February 2014 17:54, <ghi...@gmail.com <javascript:>> wrote:
>
>>
>> On Saturday, February 8, 2014 4:41:13 AM UTC, Brent wrote:
>>
>>>  On 2/7/2014 8:16 PM, ghi...@gmail.com wrote:
>>>  
>>>
>>> On Saturday, February 8, 2014 12:26:29 AM UTC, Russell Standish wrote: 
>>>>
>>>> On Fri, Feb 07, 2014 at 03:57:47PM -0800, Edgar L. Owen wrote: 
>>>> > Ghibbsa, 
>>>> > 
>>>> > Let me clarify my previous answer a little. 
>>>> > 
>>>> > P-time runs at the same intrinsic rate everywhere in the universe 
>>>> though it 
>>>> > doesn't really have a 'rate' in the usual sense since it's prior to 
>>>> > dimensionality. However that rate is the speed at which the p-time 
>>>> radial 
>>>> > dimension of the hyperspherical universe extends. That extension 
>>>> actually 
>>>> > is or produces or generates the 'flow' of p-time. 
>>>> > 
>>>>
>>>> I take it you predict that space has positive curvature (Omega > 1)? 
>>>>
>>>> Note that evidence appears to contradict this, and is widely 
>>>> considered to be the hard evidence killing Tipler's Omega point idea. 
>>>>
>>>> Or do you conceive of some method to compute this rate from a negative 
>>>> curvature? 
>>>>
>>>> Furthermore, does your theory impose an embedding dimension for the 
>>>> spacetime manifold? Because the rate at which the radial dimension 
>>>> extends is crucially dependent on the embedding dimension. 
>>>>
>>>> Note that General Relativity does not require a Euclidean embedding 
>>>> space. 
>>>>
>>>> > So p-time runs at the same intrinsic rate and provides the processor 
>>>> cycles 
>>>> > of all the computations that produce the current information state of 
>>>> the 
>>>> > universe. Part of the results of those computations are the different 
>>>> > relativistic clock time rates of processes throughout the universe. 
>>>> > 
>>>> > Hope that makes it a little clearer.... 
>>>> > 
>>>>
>>>> Not much. How do you connect the clock speed of your hypothetical 
>>>> computer with the curvature of spacetime? 
>>>>
>>>>
>>>>
>>>>   
>>> Hi Russell, I've been scratching around for ways to assemble 
>>> Edgar's case at its strongest, in terms of relativity, without actually 
>>> adding anything of my own (i.e. what he has said, just restated). 
>>>  
>>> I know this requires a stretch, maybe too far, of what you can do with a 
>>> frame in relativity. But here goes one possibility. 
>>>  
>>> Purely in the sense of how many moments there has been since the big 
>>> bang, allowing that every piece of energy in the universe (appropriately 
>>> nodding at dark energy) has its own unbroken history back to it. By 
>>> whatever measure of a 'moment' we like, shouldn't they all be resolvable in 
>>> terms of their history to the same number of moments 
>>>  
>>>
>>> NO!  If each piece of matter carried a clock along (assuming it has 
>>> indentity) they would all read differently even where they came together 
>>> because they would have traveled different spacetime paths to that 
>>> meeting.  That's why I suggested that for any given point you take the 
>>> longest interval back to the CMB and call that the time-coordinate of that 
>>> point.  And if you took a set of all such points with the same coordinate 
>>> that's a way of defining a foliation of spacetime (provided it doesn't have 
>>> any singular stuff like black holes and cosmic strings in the way).
>>>
>>> Look at Ned Wright's UCLA tutorial online.  He describes several 
>>> different ways to define a cosmic "now" (but they don't agree with each 
>>> other).
>>>
>>> Brent
>>>
>>  
>> Brent I accept that already, but would plead that you are within the 
>> relativity paradigm there, whereas the paradigm that I stated 
>> was purely historic, in which we count two moments the same, specifically 
>> and only where the same defined 'moment' counts back to the big bang at the 
>> same count. I mean, in reality there's only going to be one and exactly one 
>> same moment for each unit of energy, or not? Can the distinction you raised 
>> just there, translate into, for the history that has happened already, 
>> individual units of energy, in terms of a single number of same defined 
>> moments since the big bang, can ever have 0 of that same count, or 2 or 
>> more of that same moment? 
>>  
>> Look, I know this is potentially and very likely stepping outside what 
>> physics tells us. But what I would argue, is that by trying on edgar's 
>> ideas in the first place, if we're doing so in a reasonably well-motivated 
>> sort of way, we are already doing that. So why not let's do it right. Start 
>> by looking for how it could true most generally, which means most 
>> universally. And apply a sensible standard, which would to look for a sense 
>> first, that would be true independently of relativity, such that it too 
>> could be totally true. At least as a starting point. 
>>
>>>          
>>>
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>
>

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