Probing the cosmographic parameters to distinguish between dark energy and modified gravity models

DOI10.1051/0004-6361/200911998zbMath1253.85020arXiv0912.5141OpenAlexW1966609596WikidataQ68677532 ScholiaQ68677532MaRDI QIDQ5852088

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Publication date: 26 January 2010

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0912.5141

zbMATH Keywords

cosmology: cosmological parametersgamma rays: burstscosmology: distance scale

Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40)

Related Items (6)

A dark energy model with higher order derivatives of \(H\) in the \(f(R,T)\) modified gravity model ⋮ Anisotropic behavior of dark energy models in fractal cosmology ⋮ A study on the interacting Ricci dark energy in \(f(R,~T)\) gravity ⋮ CALIBRATION OF GRB LUMINOSITY RELATIONS WITH COSMOGRAPHY ⋮ Recovering \(\Lambda\)CDM model from a cosmographic study ⋮ Cosmological reconstruction andOmdiagnostic analysis of Einstein-Aether theory

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