kimbyd said:
The mass is the total energy in the internal degrees of freedom.
What internal degrees of freedom? As far as classical GR is concerned, a black hole doesn't have any. It just has external conserved quantities which are properties of the global geometry: mass, angular momentum, and charge.
Also see below.
kimbyd said:
These statements are true for any object, even if we don't know what the precise internal degrees of freedom are
I don't think this is valid. Before we can say a black hole's mass is the total energy in its internal degrees of freedom, I think we need, at the very least, to have some valid theory that tells us what those degrees of freedom might be. We don't have such a theory, because we don't have a valid (i.e., with at least some experimental confirmation) theory of quantum gravity. So I think the best we can say is that we would like, if possible, to find such a theory, but we don't currently have one.
Also, in GR it is not the case that the externally measured mass of an object is, in general, the total energy in its internal degrees of freedom. Unless the object is in a stationary spacetime, there is no invariant way to even specify the total energy in its internal degrees of freedom. Mass, angular momentum, and charge, as above, are external conserved quantities that are interpreted as global properties of the geometry.
kimbyd said:
The reason why the mass is the energy in the internal degrees of freedom is simply that it is the total energy of the object in that object's rest frame.
Unless that rest frame is stationary (which it isn't for any real object), this is not an invariant quantity. As an approximation, it works for a wider class of cases, but that's just an approximation.
kimbyd said:
This description is especially useful when thinking about the masses of baryons like protons and neutrons (where most of the energy is the binding energy between the quarks).
This has nothing to do with GR; all of these models are modeling the objects using QFT in flat spacetime. By construction, such a model cannot capture the interaction between the energy in the object and the spacetime geometry. But such interaction is essential for any GR model. So as far as GR is concerned, all of these models are approximations, and I don't think they come anywhere close to justifying a blanket claim about all objects, including black holes.