Interior Solutions of Fluid Sphere in f(R,T) Gravity Admitting Conformal Killing Vectors
arXiv:1610.01754 · doi:10.1007/s10509-016-2828-7
Abstract
We discuss the interior solutions of fluid Sphere in f(R,T) gravity admitting conformal killing vectors, where R is Ricci scalar and T is trace of energy momentum tensor. The solutions corresponding to isotropic and anisotropic configurations have been investigated explicitly. Further, the anisotropic case has been dealt by the utilization of linear equation of state. The results for both cases have been interpreted graphically. The equation of state parameter, integration constants and other parameters of the theory have been chosen to find the central density equal to standard value of central density of the compact objects. The energy conditions as well as stability of the solutions have been investigated in the background of f(R,T) gravity.
6 Pages, 6 Figures
References in corpus (13)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- f(R,T) gravity
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Extra force in modified theories of gravity
- Class of viable modified gravities describing inflation and the onset of accelerated expansion
- f(R,L_m) gravity
- Dark energy and dark matter as curvature effects
- Dark matter as a geometric effect in f(R) gravity
- Analysis of Rotation Curves in the framework of R^n gravity
- The matter Lagrangian and the energy-momentum tensor in modified gravity with non-minimal coupling between matter and geometry
- Generalized virial theorem in f(R) gravity
- Dark matter and dark energy as a effects of Modified Gravity
- Wormhole inspired by non-commutative geometry
Cited by in corpus (7)
- Charged Gravastars with Conformal Motion in f(R,T) Gravity
- Dynamical Analysis of Cylindrically Symmetric Anisotropic Sources in Gravity
- Kaluza-Klein bulk viscous fluid cosmological models and the validity of the second law of thermodynamics in gravity
- Self-similarity in static axially symmetric relativistic fluids
- Cosmological effects on gravity through a non-standard theory
- Collapsing scenarios of K-essence generalized Vaidya spacetime under gravity
- Cosmic evolution in the background of non-minimal coupling in Gravity