Bianchi-I dark energy cosmological model in \(f(R, L_m)\)-gravity
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Publication:6541233
DOI10.1142/S0219887824500725zbMATH Open1540.83172MaRDI QIDQ6541233
Publication date: 17 May 2024
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
- LRS Bianchi type-I universe in Barber's second self creation theory
- Constraining \(f(R)\) gravity in solar system, cosmology and binary pulsar systems
- Cosmology with curvature-saturated gravitational Lagrangian \(R/\sqrt{1 + l^4 R^2}\)
- Cosmology in scalar-tensor gravity.
- LRS Bianchi type II perfect fluid cosmological models in normal gauge for Lyra's manifold
- A class of homogeneous cosmological models
- Cosmology in \(f(R, L_m)\) gravity
- Are<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>Dark Energy Models Cosmologically Viable?
- DYNAMICS OF DARK ENERGY
- Energy conditions in f ( R , L m ) gravity
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- The cosmological constant problem
- Exact cosmological models in modified \(f(R,L_m)\) gravity with observational constraints
- Modeling transit dark energy in f(R,Lm)-gravity
- Constraints on energy conditions in \(f(R, L_m)\) gravity
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