I am wondering if the light-matter Hamiltonian obtains a dependency on the refractive index if we insert our system into a homogeneous medium that can be characterized by a scalar refractive index $n$.
Lets assume we work in the dipole approximation and treat the field classically. In this case the coupling term to a electromagnetic wave reduces to $$ H_{vac}(t) = -e \mathbf{\hat r} \cdot \mathbf E_{vac}(t)\\ \mathbf E_{vac}(t) =\boldsymbol{\epsilon} E_0\cos(\omega t) $$ where $E_0$ is the scalar amplitude of the electric field, $\boldsymbol \epsilon$ is the normalized polarization vector and $\omega$ is the angular frequency of the incident wave.
What happens in a medium with $n$ ? Are the Hamiltonians connected by a simple proportionality factor of $n$, like this $$ H_{medium}(t) \propto n^\alpha H_{vac}(t). $$ If this is appropriate, which values takes $\alpha$ and how is it derived ? How does $n$ enter the equation ?