Electromagnetic effects on the stability of anisotropic cylinder.

This paper is devoted to analyzing the stability of charged anisotropic cylinder using the radial perturbation scheme. For this purpose, we consider the non-static cylindrically symmetric self-gravitating system and apply both Eulerian as well as Lagrangian approaches to establish a linearized perturbed form of dynamical equations. The conservation of baryon number is used to evaluate perturbed radial pressure in terms of an adiabatic index. A variational principle is developed to find a characteristic frequency which helps to examine the combined effect of charge and anisotropy on the stability of gaseous star. It is found that dynamical instability can be prevented until the radius of cylinder exceeds the limit R ≥ 1 8 and anisotropy increases the instability up to the limiting value of β = − 1. 5. Finally, we conclude that the system becomes more stable by increasing the definite amount of charge gradually. [ABSTRACT FROM AUTHOR]