  We study the excited states of the Q-balls by performing stationary
perturbation on the spherical Q-balls. We find the exact solution of the
stationary perturbation of the global Q-ball with thin wall approximation. For
local Q-balls we solve the equations of motion for the perturbative part
approximately by using expansion about the coupling constant. Furthermore we
comment on the magnetic field generated by the excited Q-balls during the phase
transition precipitated by solitosyhthesis and give an implication into
cosmology.
