Compact Stars in Gravity
arXiv:2012.02587 · doi:10.1142/S0217751X21501657
Abstract
The present work is to introduce a new kind of modified gravitational theory, named as (also ) gravity, where is the Ricci scalar, is Gauss-Bonnet invariant and is the trace of the energy-momentum tensor. With the help of different models in this gravity, we investigate some physical features of different relativistic compact stars. For this purpose, we develop the effectively modified field equations, conservation equation, and the equation of motion for test particle. Then, we check the impact of additional force (massive test particle followed by a non-geodesic line of geometry) on compact objects. Furthermore, we took three notable stars named as , and . The physical behavior of the energy density, anisotropic pressures, different energy conditions, stability, anisotropy, and the equilibrium scenario of these strange compact stars are analyzed through various plots. Finally, we conclude that the energy conditions hold, and the core of these stars is so dense.
Some changes have been made. " To appear in International Journal of Modern Physics A"
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Cited by in corpus (8)
- Study of Viable Compact Stellar Structures in Non-Riemannian Geometry
- Cosmological Tests of Dark Energy Model in FRW Universe
- Charged Compact Stars in Extended Gravity
- Compact relativistic geometries in gravity
- Effects of gravity on anisotropic charged compact objects
- Some Specific Wormhole Solutions in Extended Gravity
- Energy Conditions in Extended Gravity
- Logarithm Corrections and Thermodynamics for Horndeski gravity like Black Holes