Abstract
We compute the real space galaxy power spectrum, including the leading order
effects of General Relativity and primordial non-Gaussianity from the
$f_NL$ and $g_NL$ parameters. Such contributions come
from the one-loop matter power spectrum terms dominant at large scales, and
from the factors of the non-linear bias parameter $b_NL$ (akin to
the Newtonian $b_\phi$). We use our modelling to assess the ability of
Stage-IV surveys to constrain primordial non-Gaussianity. In addition, we show
how this non-linear bias parameter can effectively renormalize diverging
relativistic contributions at large scales.
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