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I think one must be a bit careful with the notion of "vorticity". In fluid dynamics you have on the one hand a kinematic vorticity tensor related to the displacement vectors of the congruence given by the worldlines of the fluid elements and the vorticity tensor (or better circulation tensor to distinguish it from the kinematic vorticity tensor), which is a two form defined from the enthalpy current, ##w^{\mu}=h u^{\mu}##, where ##h## is the proper enthalpy density (i.e., the enthalpy density as measured in the local fluid-rest frame). The vorticity tensor then is defined by
$$\Omega_{\mu \nu}=\nabla_{\nu} w_{\mu}-\nabla_{\nu} w_{\mu}=\partial_{\nu} w_{\mu}-\partial_{\mu} w_{\nu}.$$
That's proportional to the kinematic vorticity tensor only for "dust", i.e., a pressureless fluid which is in free fall and the worldlines are thus geodesics.
Of course these quantities are in some sense frame dependent, i.e., it depends on the congruence of worldlines defined by the fluid. The distinct local frames where the physics of the tensor quantities is most easily interpreted are of course the local rest frames of the fluid, which thus is characterized by scalar quantities measured in the local rest frames of the fluid.
A very nice reference about fluid dynamics in GR is
L. Rezzolla and O. Zanotti, Relativistic hydrodynamics, Oxford University Press, Oxford (2013),
https://dx.doi.org/10.1093/acprof:oso/9780198528906.001.0001
$$\Omega_{\mu \nu}=\nabla_{\nu} w_{\mu}-\nabla_{\nu} w_{\mu}=\partial_{\nu} w_{\mu}-\partial_{\mu} w_{\nu}.$$
That's proportional to the kinematic vorticity tensor only for "dust", i.e., a pressureless fluid which is in free fall and the worldlines are thus geodesics.
Of course these quantities are in some sense frame dependent, i.e., it depends on the congruence of worldlines defined by the fluid. The distinct local frames where the physics of the tensor quantities is most easily interpreted are of course the local rest frames of the fluid, which thus is characterized by scalar quantities measured in the local rest frames of the fluid.
A very nice reference about fluid dynamics in GR is
L. Rezzolla and O. Zanotti, Relativistic hydrodynamics, Oxford University Press, Oxford (2013),
https://dx.doi.org/10.1093/acprof:oso/9780198528906.001.0001
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