Extending cosmology: the metric approach

Abstract

In this chapter it is shown how the introduction of a fundamental constant of nature with dimensions of acceleration into the theory of gravity makes it possible to extend gravity in a very consistent manner.

arXiv comment2012, Extending Cosmology: The Metric Approach, Open Questions in Cosmology; Review article for an Intech "Open questions in cosmology" book chapter (19 pages, 3 figures). Available from: http://www.intechopen.com/books/open-questions-in-cosmology/extending-cosmology-the-metric-approach

References in corpus (19)

• f(R) Theories Of Gravity
• Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• f(R,T) gravity
• Relativistic gravitation theory for the MOND paradigm
• Curvature Quintessence
• A bird's eye view of f(R)-gravity
• Wide binaries as a critical test of Classical Gravity
• The baryonic content and Tully-Fisher relation at z~0.6
• Recovering MOND from extended metric theories of gravity
• The outskirts of globular clusters as modified gravity probes
• Gravitational waves and lensing of the metric theory proposed by Sobouti
• A natural approach to extended Newtonian gravity: tests and predictions across astrophysical scales
• Understanding local Dwarf Spheroidals and their scaling relations under MOdified Newtonian Dynamics
• Flattened velocity dispersion profiles in Globular Clusters: Newtonian tides or modified gravity?
• Gravitational lensing with $f(\chi )={\chi }^{3/2}$ gravity in accordance with astrophysical observations
• A cosmological dust model with extended f(chi) gravity
• Lunar system constraints on the modified theories of gravity
• Relativistic MOND theory based on the Khronon scalar field

Cited by in corpus (1)

• Dynamics of clusters of galaxies with extended $f(\chi )$ gravity