  Tidal disruption events occur when astrophysical objects are destroyed by
black holes due to strong tidal force effects. Tidal forces have been studied
in a variety of black hole spacetimes, including Reissner-Nordstr\"om and Kerr
spacetimes. Despite the vast literature on the subject, tidal forces around
black holes in static equilibrium have never been investigated before. The aim
of this work is to fill in this gap and explore tidal forces in the
Majumdar-Papapetrou spacetime describing two extremely charged binary black
holes in equilibrium. We focus on tidal forces associated with radial and
circular geodesics of massive neutral particles moving on the plane equidistant
to the black holes. In particular, we study the behavior of the tidal forces as
a function of the distance from the black holes and as a function of the energy
of the geodesics. We also investigate the numerical solutions of the geodesic
deviation equation for different initial conditions.
