Weakly charged compact stars in f(R) gravity
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Publication:5023027
DOI10.1088/1475-7516/2018/06/006OpenAlexW2805534193MaRDI QIDQ5023027
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Publication date: 20 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1710.09294
Related Items (4)
Tideless traversable wormholes surrounded by cloud of strings in f(R) gravity ⋮ Charged quark stars in metric f(R) gravity ⋮ Models of collapsing and expanding cylindrical source in \(f(R, T)\) theory ⋮ Non violation of energy conditions in wormholes modeling
Cites Work
- Unnamed Item
- The influence of a net charge on the critical mass of a neutron star
- Beyond Einstein gravity. A survey of gravitational theories for cosmology and astrophysics.
- Structure of neutron stars in \(R\)-squared gravity
- Reissner-Nordström and charged gas spheres
- PALATINI APPROACH TO MODIFIED GRAVITY: f(R) THEORIES AND BEYOND
- Invariant Theoretical Interpretation of Interaction
- Renormalization of a Classical Gravitational Field Interacting with Quantized Matter Fields
- Sharp bounds on the radius of relativistic charged spheres: Guilfoyle's stars saturate the Buchdahl–Andréasson bound
- Junction Conditions in f(R) Theories of Gravity
- FOURTH ORDER GRAVITY: EQUATIONS, HISTORY, AND APPLICATIONS TO COSMOLOGY
- The realistic models of relativistic stars in f ( R ) = R + αR 2 gravity
- Polytropic spheres with electric charge: Compact stars, the Oppenheimer-Volkoff and Buchdahl limits, and quasiblack holes
- On Massive Neutron Cores
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