general relativity - Do non-uniformly rotating axially symmetric bodies emit gravitational waves?

In the first reply to this question it is written that:

There is no gravitational waves for a uniformly rotating axially symmetric body, because the metric doesn't depend on time.[..]

The reason is very simple. For an axially symmetric body, the distribution of mass in the lab frame coincides with that in the rotating system, thus the solution of Einstein equation can be found in the rotating system where the body and metric are static and then in the lab frame by means of r′=r, z′=z, ϕ′=ϕ+Ωt coordinate transformation (r, ϕ, z are cylindrical coordinates). Therefore all derivatives ∂xα/∂xβ do not depend on time. Hence the metric of a uniformly rotating axially symmetric body is time-independent.

So what about a non-uniformly rotating axially symmetric body?

Consider, for example, a disk rotating around its axis with a certain angular acceleration $\dot\Omega$, which could be caused by either a torque or a changing moment of inertia

In that case the metric would be time-dependent, right?

I've doubts about this because I've read about non-uniformly rotating McLaurin disks, and those seem to emit gravitational waves due to their periodic expansion/collapse cycles, not because of their non-uniform rotation.

Answer

The lowest multipole moment that needed to change to produce gravitational radiation is a quadrupole moment: $$ Q_{ij}=\int \,\rho ({\mathbf {r}})(3r_{i}r_{j}-\|{\vec {r}}\|^{2}\delta _{ij})\,d^{3}{\mathbf {r}}. $$ Energy carried away by gravitational radiation in this case is proportional to the square of third derivative of quadrupole moment: $$ -\frac{d\mathcal{E}}{dt}=\frac{G}{45 c^5} \left(\dddot{Q}_{ij}\right)^2. $$

So if the angular acceleration of a disk is caused by its changing moment of inertia tensor ($I_{ij}$) in such a way that quadrupole moment is also changing then yes, there would be gravitational radiation. Note, that not all deformations of a body would lead to a change in quadrupole moment. For example varying the radius of a massive sphere would change its moment of inertia (and if it was rotating it would change angular velocity), however quadrupole moment would remain zero and so there would be no gravitational radiation (in that order of approximation).

If however the quadrupole moment remains constant, gravitational radiation could still be generated by a changing higher multipole moment or by gravitomagnetic effects, that is changes in mass-currents while mass densities remain the same. For example if disk has inner and outer parts that could spin independently, periodically varying angular velocities of those two parts (while total angular momentum remains constant) would produce changing gravitomagnetic quadrupole moment. The power of radiation would then be proportional to the square of third derivative of gravitomagnetic quadrupole moment.

Note that in most situations contributions from gravitomagnetic multipole moments are very small.