  We derive a Higgs inflationary model in the context of holographic cosmology,
where we consider a universe filled with a Higgs field non-minimally coupled to
gravity in a slow-roll regime. The amplitude of density (scalar) perturbations
is calculated. In this regard, we show that the background and perturbative
parameters characterising the inflationary era are related to the standard one
through corrections terms. We found that for the e-fold number $N\sim 58$, the
spectral index,$n_{r}$, and the tensor-to-scalar ratio,$r$, values are $0.965$
and $0.021$, respectively, which are in agreement with 2018 Planck
observational data. However, as soon as we move from $N\sim 58$, the model is
ruled out by the current data.
