  This paper deals with the dynamics of a shearfree charged radiating collapse
in modified Gauss-Bonnet gravity. The field equations for shearfree spherical
interior geometry of a charged dissipative star are formulated. To study the
dynamical behavior of collapsing matter, we derive the dynamical as well as
transport equations. We conclude that the gravitational force in modified
Gauss-Bonnet gravity is much stronger as compared to general relativity which
implies the increase in the rate of collapse. Finally, we study the effect of
charge on the dynamics of collapse.
