Antiphon said:
But it's important to note that even the classical notions of kintetic and potential
energy are included in GR as source terms of gravitation. Spinning flywheels
gravitate more than stationary ones, the coiled sping I mentioned above, etc.
You definitely have to be careful here. Take a look at
http://math.ucr.edu/home/baez/physics/Relativity/GR/energy_gr.html
for some of the complexities of energy in full GR. You probably don't want to go around saying that GR "incorporates" classical notion of potential energy, especially gravitational potential energy as people will assume you are talking about generalized GR including cosmology, in which case the above is definitely not true.
Nonetheless, most of what you say above is reasonably close to being true in the weak-field limit of GR. In the weak-field limit, you can find the total energy (and mass, if you divide by c^2) of a *closed* system by integrating the sum of (energy density + pressure_x + pressure_y + pressure_z). This will be approximately the energy of the system - the error should be somewhere around the amount by which g_00 differs from 1 in the system under consideration. The smaller the system, the better the apprxomiation.
Objects as large as the size of our sun are still reasonably good as far as this apprxoimation goes. (The metric coefficients differs from Mikowskain flatness only in parts per million at the surface of the sun - good but but not really great as far as approximations go). When you get to cosmological scales, though, you definitely need to avoid this approximation.
Now we get to a second point:
The pressure terms will cancel out in most static systems, leaving you with the intergal of the energy density, which is in the weak-field limit equal to the energy.
While the pressure terms cancel out in _most_ systems, I'm not sure if they cancel out in rotating systems or not. One of these days I'm going to take a closer look at the rotating flywheel question, as it comes up a lot. However, even the sci.physics.faq "wimps out" on calculating the mass of a rotating flywheel.
A third point should probably be mentioned:
Finding the mass of a non-closed system is liable to give one confusing or contradictory results. I'm not sure if there is a rigorous defintion of mass that applies well to a non-closed system - the formulas I wrote above for finding the "weak-field" mass of a system probably won't work for a non-closed system, reason enough IMO to avoid non-closed systems.
A closed system would consist of (for example) a stretched spring and the bar that keeps it stretched. An open system would be a stretched spring that does not include whatever is holding it in the stretched position.
[add]
I thought of something else I should add. Having all the metric coefficients close to 1 also implies that one has a low velocity relative to the center of mass frame of the system under consideration. (The definition of "low' depends on the accuracy desired). High velocites will cause off-diagonal terms in the metric, and if they get too large the approximation starts to fail.
Reading what I wrote earlier, it's not really accurate to say that just g_00 must be close to 1 - all the metric coefficients have to be nearly Minkowskian, which means that all the on-diagonal metric coefficients must be near unity, and all the off-diagonal coefficients must be nearly zero.
The details of the justification for this approximation go like this: the nearly Minkowskian metric has a nearly timelike killing vector, thus one is in an approximately stationary space-time. This means that one can use, to a high degree of accuracy, the formulas for mass that apply to stationary space-times. There are both surface-intergal and volume intergal forms of this formula, the volume intergal forms give the result I mentioned above, that one integrates the sum of the energy and the three pressure terms over the volume. I can quote the detailed formula from Wald used if anyone is interested (one might also be able to find referenes to said formula in some of my previous posts).