Matter growth in extended ΛCDM cosmology

DOI10.1142/S021827181950086XzbMath1432.83068arXiv1706.06143MaRDI QIDQ5219545

Winfried Zimdahl, W. C. Algoner, H. E. S. Velten

Publication date: 12 March 2020

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

Full work available at URL: https://arxiv.org/abs/1706.06143

zbMATH Keywords

cosmological perturbationsscalar-tensor theoryanisotropic stressfluid cosmologymatter growth rate

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Cites Work

• Can modified gravity explain accelerated cosmic expansion?
• \(1/R\) gravity and scalar-tensor gravity
• Dark energy and dark gravity: theory overview
• Mach's Principle and a Relativistic Theory of Gravitation
• DYNAMICS OF DARK ENERGY
• Mach's Principle and Invariance under Transformation of Units

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