Dynamical Instability of Spherical Star in gravity
arXiv:1411.5676 · doi:10.1007/s10509-014-2202-6
Abstract
This work is based on stability analysis of spherically symmetric collapsing star surrounding in locally anisotropic environment in gravity, where is Ricci scalar and corresponds to the trace of energy momentum tensor. Field equations and dynamical equations are presented in the context of gravity. Perturbation schem is employed on dynamical equations to find the collapse equation. Furthermore, condition on adiabatic index is constructed for Newtonian and post-Newtonian eras to address instability problem. Some constraints on physical quantities are imposed to maintain stable stellar configuration. The results in this work are in accordance with gravity for specific case.
16 page, to appear in Astrophysics and Space Science
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- The study of Kantowski-Sachs perfect fluid cosmological model in modified gravity
- Finslerian extension of an anisotropic strange star in the domain of modified gravity
- Dissipative Cylindrical Collapse of a Charged Anisotropic Fluid in Gravity
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- Well behaved class of Heintzmann's solution within framework
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