epovo said:
It does seem however that you can have pressure with no collisions of particles.
Well - without mutual collisions in the bulk of the gas, certainly. In operational terms, however, pressure is the result of the collision of gas/liquid particles with some kind of sensor, and those most certainly do occur even in a collisionless gas. And one can generalise this to a notion of pressure at some random location in the bulk of the gas by imagining a hypothetical pressure sensor there.
My (limited) understanding is that, as Peter mentions in #8, if you cut a small cuboid out of the matter which is ##dx^\mu## on a side (I'm assuming we're using some orthonormal coordinate system here), the stress-energy tensor is what forces per unit area you have to provide on its faces so that the bulk of the matter doesn't change.
That works well for the space-space components. You can imagine putting a microscopic evacuated box into a room full of gas. The wall perpendicular to ##dx^1## must provide a force per unit area of ##p## in the ##dx^1## direction, or else the box shrinks and the volume of the gas increases slightly. A force through the ##i##th face in the ##i##th direction gives your ##T^{ii}## component. There can't be shear stresses in a gas, but you can imagine cutting a small cuboidal cavity into a stretched rubber band. Typically that would be deformed into a rhombohedron of some kind, and the ##dx^1## face would need to exert forces in the ##dx^2## and ##dx^3## directions in order to revert to its unstressed cuboid shape - and those are your ##T^{ij}##, ##i\neq j##, components.
This picture doesn't work so well for the ##T^{\mu 0}## components. It would include cutting a small break into the worldline of any matter passing though a small volume, which doesn't make sense. This is where the momentum flux explanation comes in, for me. The ##T^{i0}## components describe the amount of momentum crossing a surface due to the bulk motion of the matter in the ##dx^i## direction. In the rest frame of a material, this is zero - even in a gas where particles cross a surface, they carry equal momentum in opposite directions. But if the wind is blowing in the ##dx^i## direction,
we shall have snow then momentum flows in that direction. And finally, the ##T^{00}## component is the energy density in the volume - remember that this is a 4d volume, so it's the energy associated with particles (all on timelike trajectories, of course) in the purely timelike direction.
I think that's all correct. I must say that GR sources (at least the ones I've looked at, and I'm conscious I haven't looked in MTW yet) seem to go into far more detail on the subject of curved spacetime than on the stress-energy tensor, so this is a bit of a personal view patched together over time. Do take with a slight pinch of salt...