  We study the effect of gravity on stability of an electron living on the
3-brane. Our recently proposed fermion self-energy model is augmented by the
energy of self-gravitating electron. This energy is evaluated using the
gravitational field of a spherical source on the 3-brane derived by Garriga and
Tanaka. Owing to the smallness of the electron radius, the short-range
correction to this field dominates the Newtonian gravitational field of the
electron. The magnitude of the short-range correction is proportional to the
square of the curvature radius, $ l $, of the anti-de Sitter space. On
increasing $l$ beyond a critical value $l_{c}$, the equilibrium radius of the
electron, undergoes a transition to a region where it becomes complex-signaling
an instability of the electron. For the gravity-modified fermion self-energy
model, we find $l_{c} = 2 \times 10^{-21}$ cm. If the electron is confined by
the "hedgehog" potential, the critical length is $l_{c} = 1.6 \times 10^{-12}$
cm.
