Dark energy stars in \(f(R, G)\) gravity
From MaRDI portal
Publication:6596573
DOI10.1142/s0219887824501780zbMATH Open1546.83154MaRDI QIDQ6596573
Krishna pada Das, Ujjal Debnath
Publication date: 2 September 2024
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
- Unnamed Item
- Cosmology from \(f(R,T)\) theory in a variant speed of light scenario
- Nonperturbative models of quark stars in \(f(R)\) gravity
- Anisotropic dark energy stars
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- Singularity-free dark energy star
- Extended gravity description for the GW190814 supermassive neutron star
- Sharp bounds on the critical stability radius for relativistic charged spheres
- Probes and tests of strong-field gravity with observations in the electromagnetic spectrum
- Star models with dark energy
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
- Über das Gravitationsfeld einer Kugel aus inkompressibler Flüssigkeit nach der \textit{Einstein}schen Theorie.
- Energy conditions in modified \(f(G)\) gravity
- Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
- Energy conditions in \(f(R,G)\) gravity
- Static solutions of Einstein's field equations for spheres of fluid.
- General Relativistic Fluid Spheres
- Bounds on the basic physical parameters for anisotropic compact general relativistic objects
- Slowly rotating anisotropic neutron stars in general relativity and scalar–tensor theory
- Surface tension and negative pressure interior of a non-singular ‘black hole’
- A singularity-free solution for a charged fluid sphere in general relativity
- Anisotropic stars in general relativity
- The Maximum Mass of Ideal White Dwarfs
- Cosmological parameters from SDSS and WMAP
- On the stability of the cosmological solutions in f ( R , G ) gravity
- Gravastar: An alternative to black hole
- Role of f(G,T) gravity on the evolution of relativistic stars
- Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
- The contraction of gravitating spheres
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
- Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity
- On Massive Neutron Cores
- On Continued Gravitational Contraction
- Dark Energy Star: Physical Constraints on the Bounds
- Anisotropic strange quintessence stars in f(R,G) gravity
- Compact relativistic geometries in \(f(R, G)\) gravity
This page was built for publication: Dark energy stars in \(f(R, G)\) gravity