Stability of a Class of Non-Static Axial Self-Gravitating Systems in $f(R)$ Gravity

Abstract

In this paper, we analyze stability regions of a non-static restricted class of axially symmetric spacetime with anisotropic matter distribution. We consider $f(R)=R+\epsilon R^2$ model and assume hydrostatic equilibrium of the axial self-gravitating system at large past time. Considering perturbation from hydrostatic phase, we develop dynamical as well as collapse equations and explore dynamical instabilities at Newtonian and post-Newtonian regimes. It is concluded with the help of stiffness parameter, ${\Gamma }_1$, that radial profile of physical parameters like pressure anisotropy, energy density and higher curvature terms of the $f(R)$ model affect the instability ranges.

arXiv commentAstrophysics and Space Science, 24 pages

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• Dynamical Stability of Collapsing Stars in Einstein Gauss-Bonnet Gravity
• Dissipative Viscous Cylindrical Collapse in $f(R)$ Gravity With Full Causal Approach