  We show how one can test the cosmological Poisson equation by requiring only
the validity of three main assumptions: the energy-momentum conservation
equations of matter, the equivalence principle, and the cosmological principle.
We first point out that one can only measure the combination ${\mathcal
M}\equiv \Omega_m^{(0)}\mu$, where $\mu$ quantifies the deviation of the
Poisson equation from the standard one and $\Omega_m^{(0)}$ is the fraction of
matter density at present. Then we employ a recent model-independent forecast
for the growth rate $f(z)$ and the expansion rate $E(z)$ to obtain constraints
on ${\mathcal M}$ for a survey that approximates a combination of the Dark
Energy Spectroscopic Instrument (DESI) and Euclid. We conclude that a constant
${\mathcal M}$ can be measured with a relative error
$\sigma_{\mathcal{M}}=4.5\%$, while if ${\mathcal M}$ is arbitrarily varying in
redshift, it can be measured only to within $13.4\%$ (1 $\sigma$ c.l.) at
redshift $z=0.9$, and 15-22\% up to $z=1.5$. We also project our constraints on
some parametrizations of ${\mathcal M}$ proposed in literature, while still
maintaining model-independence for the background expansion, the power spectrum
shape, and the non-linear corrections. Generally speaking, as expected, we find
much weaker model-independent constraints than found so far for such models.
This means that the cosmological Poisson equation remains quite open to various
alternative gravity and dark energy models.
