  We consider cosmological solutions and their stability with respect to
homogeneous and isotropic perturbations in the braneworld model with the
scalar-curvature term in the action for the brane. Part of the results are
similar to those obtained by Campos and Sopuerta for the Randall-Sundrum
braneworld model. Specifically, the expanding de Sitter solution is an
attractor, while the expanding Friedmann solution is a repeller. In the
braneworld theory with the scalar-curvature term in the action for the brane,
static solutions with matter satisfying the strong energy condition exist not
only with closed spatial geometry but also with open and flat ones even in the
case where the dark-radiation contribution is absent. In a certain range of
parameters, static solutions are stable with respect to homogeneous and
isotropic perturbations.
