Quasi-homologous evolution of relativistic charged objects within \(f(\mathbf{G}, T)\) gravity
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Publication:6542239
DOI10.1016/j.cjph.2022.01.021zbMath1539.83061MaRDI QIDQ6542239
M. Z. Bhatti, Unnamed Author, Unnamed Author
Publication date: 21 May 2024
Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)
Related Items (3)
Generating fuzzy dark matter droplets ⋮ Closed time-like curves in \(f(\mathcal{R}, \mathcal{A})\) modified gravity theory ⋮ Fermion localization on the brane in Ricci-inverse gravity
Cites Work
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- Complexity and neutron star structure
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- On the \(\Lambda \)CDM universe in \(f(G)\) gravity
- Complexity and white-dwarf structure
- Modified gravity with ln \(R\) terms and cosmic acceleration
- Gauss-Bonnet gravitational baryogenesis
- Evolution of the charged dynamical radiating spherical structures
- A new type of isotropic cosmological models without singularity
- RECONSTRUCTING f(R, T) GRAVITY FROM HOLOGRAPHIC DARK ENERGY
- From Inflation to Dark Energy in the Non-Minimal Modified Gravity
- Cavity evolution in relativistic self-gravitating fluids
- Tolman mass of spherical fluids with electromagnetic field
- Cosmological parameters from SDSS and WMAP
- RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
- EXPANSION-FREE CAVITY EVOLUTION: SOME EXACT ANALYTICAL MODELS
- Role of f(G,T) gravity on the evolution of relativistic stars
- Coexistence of early-time inflation and late-time acceleration with scalar fields in theory of F(G,T) gravity
- Connecting early and late universe by f(R) gravity
- Anisotropic cosmological models in f(R,T) gravity with variable deceleration parameter
- Sur De Nouvelles Solutions Oscillatoires Des Equations De La Gravitation
- On the stability of the shear-free condition
- Role of structure scalars on the evolution of compact objects in Palatini \(f(R)\) gravity
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