On Sunday, January 6, 2019 at 12:13:16 AM UTC, Brent wrote:
>
>
>
> On 1/5/2019 1:28 PM, [email protected] <javascript:> wrote:
>
> The relation is provided by the metric.  If you choose different 
>> coordinate systems (e.g. cylindrical or spherical or whatever) then there 
>> is different metric tensor.  So the integral along the path of g_ab dx^a 
>> dx^b is the same.
>>
>> Brent
>>
>
> *I assume you're showing why the proper time along a given path is the 
> same for all observers, and this has nothing to do with coordinate time 
> being unrelated to proper time. AG *
>
>
> Coordinate time between events A and B is just delta(x^0) = x^0(B) - 
> x^0(A).  Just like the longitudinal distance between LA and NY is 
> Long(LA)-Long(NY).  But the driving distance between LA and NY depends on 
> the path you take and is an integral along that path which includes changes 
> in latitude:
>
>     S^2 = INT_path g_ab dx^a dx^b = INT_path [ dlong*dlong*cos^2(lat) + 
> dlat*dlat]
>
> Notice the cos^2 factor because the space isn't  flat.   
>
> So in GR coordinate time is related to proper time; it contributes a term 
> in accordance with the metric that describes the curvature of the 
> spacetime.  But there are other terms from the spatial coordinates and even 
> cross terms and the terms are weighted by the metric factors that describe 
> the shape of the space.
>
> Brent
>

*I think you mean that coordinate time is related to proper time as a path 
is traversed, even though elapsed coordinate time is the same for all paths 
having the same initial and endpoints in spacetime. AG *

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