The spatial stress is a two-index, symmetric tensor, and the only objects that can be used to carry the indices are the four-velocity and the metric . Furthermore, because the spatial stress must also be symmetric, the only possibility is a linear combination of and . Given that , we find

As the system is assumed to be locally isotropic, it is possible to diagonalize the spatial-stress tensor. This also implies that its three independent diagonal elements should actually be equal to the same quantity, which is the local pressure. Hence we have and which is the well-established result for a perfect fluid.Given a relation , there are four independent fluid variables. Because of this the equations of motion are often understood to be , which follows immediately from the Einstein equations and the fact that . To simplify matters, we take as equation of state a relation of the form where is the particle number density. The chemical potential is then given by

and we see from the Euler relation (79) thatLet us now get rid of the free index of in two ways: first, by contracting it with and second, by projecting it with (letting ). Recalling the fact that we have the identity

Contracting with and using this identity gives The definition of the chemical potential and the Euler relation allow us to rewrite this as where . Projection of the free index using leads to where is a purely spatial derivative and is the acceleration. This is reminiscent of the familiar Euler equation for Newtonian fluids.However, we should not be too quick to think that this is the only way to understand . There is an alternative form that makes the perfect fluid have much in common with vacuum electromagnetism. If we define

and note that , then The stress-energy-momentum tensor can now be written in the form We have here our first encounter with the fluid element momentum that is conjugate to the particle number density current . Its importance will become clearer as this review develops, particularly when we discuss the two-fluid case. If we now project onto the free index of using , as before, we find where the force density is and the vorticity is defined as Contracting Equation (101) with implies (since ) that and as a consequence The vorticity two-form has emerged quite naturally as an essential ingredient of the fluid dynamics [72, 19, 11, 60]. Those who are familiar with Newtonian fluids should be inspired by this, as the vorticity is often used to establish theorems on fluid behavior (for instance the Kelvin–Helmholtz theorem [66]) and is at the heart of turbulence modeling [93].To demonstrate the role of as the vorticity, consider a small region of the fluid where the time direction , in local Minkowski coordinates, is adjusted to be the same as that of the fluid four-velocity so that . Equation (105) and the antisymmetry then imply that can only have purely spatial components. Because the rank of is two, there are two “nulling” vectors, meaning their contraction with either index of yields zero (a condition which is true also for vacuum electromagnetism). We have arranged already that be one such vector. By a suitable rotation of the coordinate system the other one can be taken as , thus implying that the only non-zero component of is . “MTW” [80] points out that such a two-form can be pictured geometrically as a collection of oriented worldtubes, whose walls lie in the and planes. Any contraction of a vector with a two-form that does not yield zero implies that the vector pierces the walls of the worldtubes. But when the contraction is zero, as in Equation (105), the vector does not pierce the walls. This is illustrated in Figure 6, where the red circles indicate the orientation of each world-tube. The individual fluid element four-velocities lie in the centers of the world-tubes. Finally, consider the closed contour in Figure 6. If that contour is attached to fluid-element worldlines, then the number of worldtubes contained within the contour will not change because the worldlines cannot pierce the walls of the worldtubes. This is essentially the Kelvin–Helmholtz theorem on conservation of vorticity. From this we learn that the Euler equation is an integrability condition which ensures that the vorticity two-surfaces mesh together to fill out spacetime.

As we have just seen, the form Equation (105) of the equations of motion can be used to discuss the conservation of vorticity in an elegant way. It can also be used as the basis for a derivation of other known theorems in fluid mechanics. To illustrate this, let us derive a generalized form of Bernoulli’s theorem. Let us assume that the flow is invariant with respect to transport by some vector field . That is, we have

Here one may consider two particular situations. If is taken to be the four-velocity, then the scalar represents the “energy per particle”. If instead represents an axial generator of rotation, then the scalar will correspond to an angular momentum. For the purposes of the present discussion we can leave unspecified, but it is still useful to keep these possibilities in mind. Now contract the equation of motion (105) with and assume that the conservation law Equation (104) holds. Then it is easy to show that we have In other words, we have shown that is a conserved quantity.Given that we have just inferred the equations of motion from the identity that , we now emphatically state that while the equations are correct the reasoning is severely limited. In fact, from a field theory point of view it is completely wrong! The proper way to think about the identity is that the equations of motion are satisfied first, which then guarantees that . There is no clearer way to understand this than to study the multi-fluid case: Then the vanishing of the covariant divergence represents only four equations, whereas the multi-fluid problem clearly requires more information (as there are more velocities that must be determined). We have reached the end of the road as far as the “off-the-shelf” strategy is concerned, and now move on to an action-based derivation of the fluid equations of motion.

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