On Sunday, July 12, 2020 at 4:37:15 PM UTC-6, Lawrence Crowell wrote:
>
> I have not followed this thread much. I get the impression there is a lot 
> of confusion. 
>
> The equivalence principle states there is no distinguishing difference 
> between a frame far away in flat spacetime and one in a region of spacetime 
> that is curved so long as the frame is small in extent. In other words, it 
> there is a curvature R and the dimensions of the frame are d then d << √R. 
> This will mean that any test masses in this small frame will be on 
> co-parallel geodesics and the local physics is no different than if you are 
> on a frame in very distant flat spacetime. The converse of this then is 
> that being on an accelerated frame is indistiguishable from being held 
> fixed in a gravitational field. The surface of the Earth does that for us. 
> Then comparing gravity with acceleration this way the implication is that 
> inertial mass is equal to gravitational mass. The previous case indicates a 
> way forwards to general relativity with local frames or patches that are 
> meshed together in a coordinate atlas and transition function that define 
> connection coefficients and curvature.
>
> What you write above is not substantially different from my description of 
the EP. AG
 

> Is there a better way to do this, Yes! this is what I have been working 
> on. Instead of a single small inertial frame consider two frames and in 
> each there is one of each EPR pair, The easy part is to show that the 
> entanglement is constant so long as the two frames are on geodesic motion. 
> This is a sort of extended EP which is potentially useful for quantum 
> gravitation. This is in particular if spacetime is built up from quantum 
> entangled states. Things becomes much more difficult when black hole 
> horizons enter the picture. 
>
> The standard EP is not that hard to understand, and in weak gravitation 
> the obvious example of this are weightless objects and astronauts in 
> spacecraft and the ISS. In effect this is moving horizontally fast enough 
> to keep missing the Earth and it just keeps falling. This is a visual 
> example of the EP.
>
> LC
>

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