Chaplygin-gas solutions of f(R) gravity
DOI10.1142/S0219887816501206zbMath1355.83035arXiv1603.05535OpenAlexW2296916791MaRDI QIDQ3179749
Maye Elmardi, Amare Abebe, Abiy Tekola
Publication date: 20 December 2016
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1603.05535
cosmologyChaplygin gasdark matterdark energy\(f(R)\) gravitydark energy-driven late-time cosmic accelerationscalar field-driven early universe expansion (inflation)
Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)
Related Items (6)
Cites Work
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- Metric-affine \(f(R)\) theories of gravity
- Palatini \(f(R)\) gravity as a fixed point
- Generalized Chaplygin gas model: dark energy -- dark matter unification and CMBR con\-straints
- Kinematics and dynamics of \(f(R)\) theories of gravity
- Breaking the cosmological background degeneracy by two-fluid perturbations in f(R) 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
- Irrotational-fluid cosmologies in fourth-order gravity
- The universe dominated by the extended Chaplygin gas
- Structure growth in f ( R ) theories of gravity with a dust equation of state
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