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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 togravity in a slow-roll regime. The amplitude of density (scalar) perturbationsis calculated. In this regard, we show that the background and perturbativeparameters characterising the inflationary era are related to the standard onethrough corrections terms. We found that for the e-fold number $N\sim 58$, thespectral index,$n_{r}$, and the tensor-to-scalar ratio,$r$, values are $0.965$and $0.021$, respectively, which are in agreement with 2018 Planckobservational data. However, as soon as we move from $N\sim 58$, the model isruled out by the current data.

Non-minimal Higgs inflation within holographic cosmology