A Modified Gravity and its Consequences for the Solar System, Astrophysics and Cosmology
arXiv:gr-qc/0608074 · doi:10.1142/S0218271807011577
Abstract
A relativistic modified gravity (MOG) theory leads to a self-consistent, stable gravity theory that can describe the solar system, galaxy and clusters of galaxies data and cosmology.
16 pages. Latex file. Talk given at the International Workshop "From Quantum to Cosmos: Fundamental Physics in Space", 22-24 May, 2006, Warrenton, Virginia, USA. To be published in Int. J. Mod. Phys D. Equation corrected
References in corpus (8)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Tests of the Gravitational Inverse-Square Law
- Study of the anomalous acceleration of Pioneer 10 and 11
- Galaxy Rotation Curves Without Non-Baryonic Dark Matter
- A New Nucleosynthesis Constraint on the Variation of G
- Testing the Newton law at long distances
- Dark Matter Searches
Cited by in corpus (15)
- Testing modified gravity with globular cluster velocity dispersions
- Constraining the range of Yukawa gravity interaction from S2 star orbits
- Weak gravitational lensing by Kerr-MOG Black Hole and Gauss-Bonnet theorem
- Particle Dynamics Near Kerr-MOG Black Hole
- The bending of light and lensing in modified gravity
- Constraining the range of Yukawa gravity interaction from S2 star orbits III: improvement expectations for graviton mass bounds
- Circular Motion and Energy Extraction in a Rotating Black Hole
- On the universality of MOG weak field approximation at galaxy cluster scale
- Exact cosmological solutions for MOG
- Gravitational synchrotron radiation and Penrose process in STVG theory
- Perturbations of Keplerian Orbits in Stationary Spherically Symmetric Spacetimes
- New Constraints on Dark Matter and Cosmic Neutrino Profiles through Gravity
- Scalar-tensor black holes in an expanding universe
- Dark Coincidences: Small-Scale Solutions with Refracted Gravity and MOND
- Local Stability of Galactic Discs in Modified Dynamics