  Tidal forces produced by black holes are an important result of General
Relativity, related to the spacetime curvature tensor. Among the astrophysical
implications of tidal forces, stands out tidal disruption events. We analyze
the tidal forces in the spacetime of an electrically charged Hayward regular
black hole, obtaining the components of the tidal tensor and the geodesic
deviation equation. We find that the radial and angular tidal forces may vanish
and change sign, unlike in the Schwarzschild spacetime. We note that tidal
forces are finite at the origin of the radial coordinate in this regular black
hole spacetime. We obtain the geodesic deviation vector for a body constituted
of dust infalling towards the black hole with two different initial conditions.
