  It has been suggested by Weinberg et al. (2013) that an instability due to
the nonlinear coupling of a neutron star's tide to its $p$- and $g$-modes could
affect the gravitational-wave phase evolution of a neutron-star binary.
Weinberg (2016) suggests that this instability can turn on as the
gravitational-waves pass through the sensitive band of ground-based detectors,
although the size of the effect is not known. The discovery of the binary
neutron star merger GW170817 provides an opportunity to look for evidence of
nonlinear tides from $p$-$g$ mode coupling. We compute Bayesian evidences that
compare waveform models that include the $p$-$g$ mode coupling to models that
do not. Using the waveform model and priors of Essick et al. (2016) we find
that the observation of GW170817 is consistent with $p$-$g$ mode coupling, in
agreement with Abbott, B. P., et al. (2019a). We investigate the properties of
the model and find that this consistency is due to degeneracy in a large region
of the parameter space between the the model that includes nonlinear tides from
$p$-$g$ mode coupling and the standard post-Newtonian model that does not. We
investigate the consistency of the GW170817 signal with regions of the
parameter space where the effect of nonlinear tides is not degenerate with the
standard model. Regions of the nonlinear tide parameter space that have a
fitting factor of less than 99$\%$ (98.5$\%$) are disfavored by a Bayes factor
of 15 (25). We conclude that the consistency of the GW170817 signal with the
model of Essick et al. (2016) is due to parameter degeneracy and that regions
where nonlinear tides produce a measurable effect are strongly disfavored.
