MOND and cosmology

R. H. Sanders*

*Bijbehorende auteur voor dit werk

OnderzoeksoutputAcademicpeer review

4 Citaten (Scopus)

Samenvatting

I review various ideas on MOND cosmology and structure formation beginning with non-relativistic models in analogy with Newtonian cosmology. I discuss relativistic MOND cosmology in the context of Bekenstein's theory and propose an alternative biscalar effective theory of MOND in which the acceleration parameter, a(0) is identified with the cosmic time derivative of a matter coupling scalar field and cosmic CDM appears as scalar field oscillations of the auxiliary "coupling strength" field.

Originele taal-2English
TitelMass Profiles and Shapes of Cosmological Structures
RedacteurenGA Mamon, F Combes, C Deffayet, B Fort
Plaats van productieCEDEX A
UitgeverijE D P SCIENCES
Pagina's231-238
Aantal pagina's8
ISBN van geprinte versie2-86883-917-7
DOI's
StatusPublished - 2006
Evenement21st IAP Colloquium on Mass Profiles and Shapes of Cosmological Structures - , France
Duur: 4-jul.-20059-jul.-2005

Publicatie series

NaamEAS PUBLICATIONS SERIES
UitgeverijE D P SCIENCES
Volume20
ISSN van geprinte versie1633-4760

Other

Other21st IAP Colloquium on Mass Profiles and Shapes of Cosmological Structures
Land/RegioFrance
Periode04/07/200509/07/2005

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