pmb_phy said:
If the object is extended object then its more commplicated.
Note Pressure contributes to inertia. E.g. see Shutz's new text Gravity from the ground up. Especially at the bottom of page 192 in the section entitled The extra inertia of pressure.
I don't have the text (though I hear it's quite good) - but you are right that pressure contributes to the stress energy tensor and hence the mass of a system.
Defining the mass of an extended system as the response to an external force is however an extremely bad idea, just because of the very fact that the mass of the system does depend on the distribution of the stresses. This means that different force distributions give different masses, an unsavory state of affairs. Fortunately, there are MUCH better ways of defining the mass of an extended system than considering the response of a system to an external force. More on this later.
Sorry lad but I didn't correct anybody in this thread. I stated my opinion that writing m = E/c^2 is bad juju.
There's no accounting for taste. Most peole learned SR wrong.
Pete
E = mc^2 is perfectly fine as long as p (momentum!) is zero, and m is invariant mass. (Apparently you did nor realize that p was momentum? Or were you pulling my leg? I think you were pulling my leg - though I doubt you'll admit it.)
Thus there's no reason for people to un-learn E=mc^2, all they have to do is realize that that equation only works when p=0, and that the real equation is more like E^2 - (pc)^2 = (mc^2)^2, (when p is not zero), which can be further simplfied by using geometric units to E^2 - p^2 = m^2. And they need to know that the m in this equation is the "invariant mass".
In addition, people eventually have to learn that the total energy E of a system is not the intergal of the energy density term of the stress-energy tensor (T_00), but also does includes contribution from the pressure terms as you state.
However, given that one has the necessary condtions - an isolated system and an
asymptotically flat space-time will do, the resulting system has a well defined energy E in GR, and a well defined momentum p, as well. One confusing thing is that the energy of the extended system is not just the intergal of the energy density, but includes the intergal of some of the pressure terms as well. Note well that with these (standard!) defintions of energy and momentum, in geometric units E^2 - p^2 = m^2 works for both point particles AND extended systems.
Given that a system has an energy E and a momentum P, and that these quantities transform as a 4-vectors in the appropriate
asymptotically flat space-time (which they do), it's trivial to compute the invariant mass 'm' of the system, usually just called the mass. If one needs to be especially precise, the mass of a system can be sub-categorized into at least two types of mass - the ADM mass, and the Bondi mass. The ADM mass is mathematically based on the behavior of the system at space-like infinity, and includes gravitational radiation terms. The Bondi mass is mathematically based on the behavior of the system at null infinity, and does not include gravitational radiation contributions.
Usually such detail is not needed or even wanted at the introductory level. The best source for information on mass in GR is probably Wald's "General Relativity", which is not an introductory book.