In the paper Asymptotic Time Behavior of Correlation Functions (1970), the authors study the time behaviour of the velocity-velocity correlation function of a particle in a gas. If the gas is in $d$ spatial dimensions, they find that
$$ C(t)=\frac{\langle v(0)_i v(t)_i \rangle}{\langle v(0)_i^2 \rangle} \sim t^{-d/2} $$
where the average refers to an equilibrium ensemble. Therefore, they conclude that the self-diffusion coefficient $D$ does not exist when $d=2$, so that "conventional hydrodynamics does not exist in two dimensions". This is because, thanks to the Green-Kubo formula,
$$ D \propto \int_0^{\infty} C(t) \, dt $$
the diffusion coefficient $D$ is logarithmically divergent for $d=2$.
Is this a well-known result? Does it imply that we can not apply Navier stokes for a gas in two dimensions? (i.e. interacting particles constrained on a surface can not be described in the long-wavelength limit by Navier-Stokes hydrodynamics).
Moreover, the authors of Velocity-Correlation Functions in Two and Three Dimensions: Low Density (1972) write: Physically the long-time tails $~1/t$ of the correlation functions are caused by the slowly decaying hydrodynamic modes. Kinetically, this is due to the possibility of recollisions, i.e., collisions between two particles that have collided before. They lead to a much slower decay of the initial state of a particle than if they are excluded since they can still "remind" the particle of its initial state after many collisions have taken place.
These two papers are from the '70s, which is the situation today? Can we apply Navier Stokes (or the diffusion equation) when $d=2$ and $d=1$?
Note: Of course, Navier-Stokes works in $d=2$, in the sense that it can be solved (see this answer). My question is whether Navier-Stokes can be justified from a kinetic perspective. While for $d>2$, we can derive it from kinetic theory, what about for $d<3$?
Note: Interestingly, even the Boltzmann equation seems to be problematic for some $d=2$ fluid models, see this answer.