If a differential operator is a linear map and has nonzero kernel of a linear map, the equation determines only up to a homogeneous solution. Lorentz covariance of and therefore does not force independently selected solutions in different inertial frames to obey a particular tensor transformation law. A covariant Green function and consistently transformed homogeneous data do provide such a choice. For the four-potential in Lorenz gauge, still permits with , a residual Lorenz gauge symmetry. Constant spatial potentials for zero sources are a concrete example.
A physical quantity is Lorentz invariant when its value is unchanged under Lorentz transformations. Tensor equations can be Lorentz covariant while their components transform. Fixed-vector gauge choices need not make covariance manifest, although physical gauge-invariant predictions retain the symmetry.
Dynamical equations whose solutions transform into solutions under a Lorentz transformation, holding fixed the theory's physical background data. A scalar matter equation constructed from the Minkowski metric has this property; introducing a preferred timelike vector field into the matter equation can destroy it.
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Lorentz covariance is a fundamental principle in the theory of relativity that describes how the laws of physics remain invariant under Lorentz transformations, which relate the coordinates of events as observed in different inertial reference frames moving at constant velocities relative to each other. In more detail, Lorentz transformations include combinations of rotations and boosts (changes in velocity) that preserve the spacetime interval between events.
Same motivation as Galilean invariance, but relativistic version of that: we want the laws of physics to have the same form on all inertial frames, so we really want to write them in a way that is Lorentz covariant.
This is just the relativistic version of that which takes the Lorentz transformation into account instead of just the old Galilean transformation.