Anisotropic universe in \(f(\mathcal{G}, T)\) gravity
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Publication:1708827
DOI10.1155/2017/6378904zbMath1383.83240arXiv1705.05729OpenAlexW3123082451MaRDI QIDQ1708827
Publication date: 27 March 2018
Published in: Advances in High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1705.05729
Relativistic cosmology (83F05) Topological field theories in quantum mechanics (81T45) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (5)
Bianchi I metric solutions with nonminimally coupled Einstein-Maxwell gravity theory ⋮ Energy bounds in f(R,G) gravity with anisotropic background ⋮ Plane symmetric solutions in \(f(\mathcal{G}, T)\) gravity ⋮ $f({\mathcal{G}},T)$ Gravity with Cylindrically Symmetric Relativistic Fluids ⋮ The impact of f(G,T) gravity on the evolution of cavity in the cluster of stars
Cites Work
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- A new type of isotropic cosmological models without singularity
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- Built-in inflation in f(G) gravity
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- Wormholes supported by f(𝒢) gravity
- Some exact solutions in f(𝒢,T) gravity via Noether symmetries
- Dark energy problem: from phantom theory to modified Gauss–Bonnet gravity
- Exact solutions of Bianchi-type I and V spacetimes in the f ( R ) theory of gravity
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