Impact of \(f(\mathrm{R},\varphi,\chi)\) theory on the geometry of charged stellar objects
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Publication:6550870
DOI10.1016/j.aop.2024.169674zbMATH Open1540.8311MaRDI QIDQ6550870
Publication date: 5 June 2024
Published in: Annals of Physics (Search for Journal in Brave)
stability analysisanisotropic fluidscalar-tensor theorycompact star\(f(\mathrm{R},\varphi,\chi)\) gravity
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15)
Cites Work
- Anisotropic stars. II: Stability
- Dark \(f(\mathcal{R},\varphi,\chi)\) universe with Noether symmetry
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- Stable dark energy stars
- CHARGED ANALOGUE OF FINCH–SKEA STARS
- CURVATURE QUINTESSENCE
- Stellar structures admitting Noether symmetries in f(ℛ,𝒯 ) gravity
- Higher dimensional charged compact objects in Finch–Skea geometry
- Dynamics of perfect fluid collapse in f(𝒢,T) gravity
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- New exact spherically symmetric solutions in f(R,ϕ,X) gravity by Noether's symmetry approach
- Study of Charged Anisotropic Karmarkar Stars in f(R,T2)$f(\mathcal {R},\mathbb {T}^{2})$ Theory
- Anisotropic compact stars with karmarkar condition in energy-momentum squared gravity
- Study of stellar structures in f(ℛ,𝒯μν𝒯μν) theory
- Dynamics of cylindrical collapse in \(f(\mathcal{G}, T )\) gravity
- Dynamics of charged anisotropic spherical collapse in energy-momentum squared gravity
- Anisotropic compact stars admitting Karmarkar condition in \(f(\mathcal{Q})\) theory
- Charged spherical solution in \(f(G, T)\) gravity via embedding
- Scalar field cosmology via Noether symmetries in energy-momentum squared gravity
- Viable and stable compact stellar structures in \(f(\mathcal{Q}, \mathcal{T})\) theory
- Viable wormhole solutions in modified Gauss-Bonnet gravity
Related Items (2)
Exploring Gauss Bonnet gravity in the realm of Tolman-Kuchowicz spacetime ⋮ Investigation of Bardeen stellar structures in modified \(f(R, \phi, X)\) theory of gravity
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