Study of a quadratic redshift-based correction in f(R) gravity with Baryonic matter

DOI10.1142/S0218271815500911zbMath1332.83011OpenAlexW2221361003MaRDI QIDQ2791781

Mozhgan Masoudi, Reza Saffari

Publication date: 16 March 2016

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0218271815500911

zbMATH Keywords

cosmologymodified gravitysemi-inverse method

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05)

Related Items (1)

Solar system tests of a new class of f(z) theory

Cites Work

• \(1/R\) gravity and scalar-tensor gravity
• Cosmological constant -- the weight of the vacuum
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Vacuum solution of a linear red-shift based correction in \(f (R)\) gravity
• DYNAMICS OF DARK ENERGY
• CURVATURE QUINTESSENCE
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Cosmological dynamics of R ⁿ gravity

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