We present a covariant framework to compute scattering amplitudes and
potentials in a de Sitter background. In this setting, we compute the
potential of a graviton-mediated scattering process involving two very
massive scalars at tree level. Although the obtained scattering
potential reproduces the Newtonian potential at short distances, on
Hubble-size length scales it is affected by the constant curvature:
effectively, it yields a repulsive force at sub-Hubble distances. This
can be attributed to the expansion of the de Sitter universe. Beyond the
de Sitter horizon, the potential vanishes identically. Hence, the
scattering amplitude unveils the geometric properties of de Sitter
spacetime in a novel and nontrivial way.