  The entanglement entropy of the event horizon is known to be plagued by the
UV divergence due to the infinitely blue-shifted near horizon modes. In this
paper we calculate the entanglement entropy using the transplanckian dispersion
relation, which has been proposed to model the quantum gravity effects. We show
that, very generally, the entropy is rendered UV finite due to the suppression
of high energy modes effected by the transplanckian dispersion relation.
