Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-20T00:35:08.380Z Has data issue: false hasContentIssue false
  • English
  • Français

MOND and Cosmology

Published online by Cambridge University Press:  19 May 2006

G.A. Mamon ,
F. Combes ,
C. Deffayet ,
B. Fort  and
R.H. Sanders
R.H. Sanders*
Affiliation:
Kapteyn Astronomical Institute, PO Box 800, 9700 AV Groningen, The Netherlands
Get access

Abstract

I review various ideas on MOND cosmology and structureformationbeginning with non-relativistic models in analogy with Newtonian cosmology. I discuss relativistic MOND cosmology in the context ofBekenstein's theory and propose an alternative biscalar effective theoryof MOND in which the acceleration parameter, a0 is identifiedwith the cosmic time derivative of a matter coupling scalar fieldand cosmic CDM appears as scalar field oscillations of theauxiliary “coupling strength” field.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 20: Mass Profiles and Shapes of Cosmological Structures , 2006 , pp. 231 - 238
Copyright
© EAS, EDP Sciences, 2006

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)