Modified Gravity and its Consequences for the Solar System, Astrophysics and Cosmology
APA
Moffat, J. (2007). Modified Gravity and its Consequences for the Solar System, Astrophysics and Cosmology. Perimeter Institute. https://pirsa.org/07050045
MLA
Moffat, John. Modified Gravity and its Consequences for the Solar System, Astrophysics and Cosmology. Perimeter Institute, May. 20, 2007, https://pirsa.org/07050045
BibTex
@misc{ pirsa_PIRSA:07050045, doi = {10.48660/07050045}, url = {https://pirsa.org/07050045}, author = {Moffat, John}, keywords = {Cosmology}, language = {en}, title = {Modified Gravity and its Consequences for the Solar System, Astrophysics and Cosmology}, publisher = {Perimeter Institute}, year = {2007}, month = {may}, note = {PIRSA:07050045 see, \url{https://pirsa.org}} }
Perimeter Institute for Theoretical Physics
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Abstract
A relativistic modified gravity (MOG) leads to a self-consistent, stable gravity theory that can describe the solar system, galaxy and clusters of galaxies data and cosmology without dark matter. A review is given of fits to galaxy rotation curves, mass profiles of X-ray clusters and weak and strong lensing of galaxy clusters including the bullet cluster E10657-56. MOG can explain the CMB power spectrum and the observed acceleration of the expansion of the universe.