Large scale density perturbations from a uniform distribution by wave
  transport
  It has long been known that a uniform distribution of matter cannot produce a
Poisson distribution of density fluctuations on very large scales $1/k > ct$ by
the motion of discrete particles over timescale $t$. The constraint is part of
what is sometimes referred to as the Zel'dovich bound. We investigate in this
paper the transport of energy by the propagation of waves emanating {\it
incoherently} from a regular and infinite lattice of oscillators, each having
the same finite amount of energy reserve initially. The model we employ does
not involve the expansion of the Universe -- the scales of interest are all
deeply sub-horizon -- but the size of regions over which perturbations are
evaluated far exceed $ct$, where $t$ is the time elapsed since the start of
emission (it is assumed that $t$ greatly exceeds the duration of emission). We
find that to lowest order, when only wave fields $\propto 1/r$ are included,
there is exact compensation between the energy loss of the oscillators and the
energy emitted into space, which means $P(0)=0$ for the power spectrum of
density fluctuations on the largest scales. This is consistent with the
Zel'dovich bound. To the next order when near fields $\propto r^{-2}$ are
included, however, $P(0)$ settles at late times to a positive value that
depends only on time, as $t^{-2}$ (the same applies to an energy non-conserving
term). Even though this effect looks like superluminal energy transport, there
is no violation of causality because the two-point function vanishes completely
for $r>t$ if the emission of each oscillator is truncated beyond some duration.
The result calls to question any need of enlisting cosmic inflation to seed
large scale density perturbations. When applied to fast radio bursts --
uniformly distributed transients (to lowest order) that repeat at other
locations -- the result supports Hoyle's hypothesis of constant energy
injection.
