arXiv · 1405.1378
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 $f(R)=R+εR^2$ 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, $Γ_1$, that radial profile of physical parameters like pressure anisotropy, energy density and higher curvature terms of the $f(R)$ model affect the instability ranges.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
M. Sharif, Z. Yousaf. 2014-06-03. Stability of a Class of Non-Static Axial Self-Gravitating Systems in $f(R)$ Gravity. https://doi.org/10.1007/s10509-014-1985-9
Cite the original work for its findings. Save a collection to share your selection of sources.