The reverse Burnett conjecture for null dusts

Given a regular solution ${\mathbf{g}}_0$ of the Einstein-null dusts system without restriction on the number of dusts, we construct families of solutions $({\mathbf{g}}_{\lambda }{)}_{\lambda \in (0,1]}$ of the Einstein vacuum equations such that ${\mathbf{g}}_{\lambda }-{\mathbf{g}}_0$ and $\mathrm{\partial }({\mathbf{g}}_{\lambda }-{\mathbf{g}}_0)$ converges respectively strongly and weakly to 0 when $\lambda \to 0$. Our construction, based on a multiphase geometric optics ansatz, thus extends the validity of the reverse Burnett conjecture without symmetry to a large class of massless kinetic spacetimes. In order to deal with the finite but arbitrary number of direction of oscillations we work in a generalised wave gauge and control precisely the self-interaction of each wave but also the interaction of waves propagating in different null directions, relying crucially on the non-linear structure of the Einstein vacuum equations. We also provide the construction of oscillating initial data solving the vacuum constraint equations and which are consistent with the spacetime ansatz.