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2.3 The Hydrodynamic Equations<br />
In local equilibrium, the conditions of Eqs(27) are not met, and the left hand<br />
sides (that we shall call thermodynamic forces) are not zero. This leads to<br />
dissipative terms (denoted below by the superscript D ) and entropy production<br />
as functions of the thermodynamic forces, which parameterize the deviation<br />
from global equilibrium. The variables of course still obey continuity equations,<br />
with<br />
0=∂t(B + B D )+c ∇×(E + E D ) ,<br />
0=∂t(D + D<br />
(30)<br />
D )+j D el +(ρel + ρ D el) v<br />
−c ∇×(H + H D ) , (31)<br />
0=∂t(ρ + ρ D )+∇·(ρ v − j D ) , (32)<br />
0=∂t(ρc + ρ D c )+∇·(ρc v − j D c ) , (33)<br />
R/T = ∂t(s + s D )+∇·(s v − f D ) , (34)<br />
0=∂t (g tot<br />
i + g tot,D<br />
i )+∇j (Πij − Π D ij) , (35)<br />
0=∂t(ɛ tot + ε D )+∇·(Q + Q D ) (36)<br />
∇·(B + B D )=0, (37)<br />
∇·(D + D D )=ρel + ρ D el . (38)<br />
We may subtract the equation of motion for mass from that of the total energy<br />
ɛ tot , to arrive at the continuity equation for the non-relativistic form of energy<br />
conservation, more usual in hydrodynamic theories,<br />
0=∂t(ε + ε D − ρ D c 2 )+∇·(Q + Q D<br />
−ρc 2 v + c 2 j D ) . (39)<br />
The covariance of the Eqs(30 - 38) has a number of consequences:<br />
• The equilibrium contributions of energy, momentum and their fluxes constitute<br />
the equilibrium energy-momentum 4-tensor Π µν ; the same applies<br />
to the nonequilibrium contributions, ε D , Q D , g tot,D and −Π D ij constitute the<br />
nonequilibrium 4-tensor Π D,µν .<br />
• Analogously, all fields, the equilibrium and nonequilibrium ones, (E, B),<br />
(E D , B D ), (D, H) and (D D , H D ) constitute 4-tensors of the form<br />
8