Cavediver,I have a question about GR and didn't want to start a new thread, so I'll post it here. I'm sure you can answer it easily.
In GR, the curveture of spacetime, expressed as excess radius of a sphere, is given by the formula:
Radius excess= (GM)/(3c^2)
(This is according to Feynman's "Six Not So Easy Pieces", though in the preface it's noted that he leaves out the sum of the pressures in this statement.)
Then, it's stated that this excess radius will be independent of frames of reference. How is this so, since mass is dependent on the frame of reference?
My guess is that although the frames of reference will get a different mass, they are using different coordinate systems, and in their coordinate system they will get the same excess radius. Is this correct?