  In this paper, we study the cracking of compact object PSR J1614-2230 in
quadratic regime with electromagnetic field. For this purpose, we develop a
general formalism to determine the cracking of charged compact objects. We
apply the local density perturbations to the hydrostatic equilibrium equation
as well as all the physical variables involve in the model. We plot the force
distribution function against radius of the star with different values of model
parameters both with and without charge. It is found that PSR J1614-2230
remains stable (no cracking) corresponding to different values of parameters
when charge is zero, while it exhibit cracking (unstable) when charge is
introduced. We conclude that stability region increases as amount of charge
increases.
