A Possible Late Time $Λ$CDM-like Background Cosmology in Relativistic MOND Theory

Details A Possible Late Time $Λ$CDM-like Background Cosmology in Relativistic MOND Theory A Possible Late Time $Λ$CDM-like Background Cosmology in Relativistic MOND Theory

2005-04-05

arxiv.org/abs/astro-ph/0504130v3

Int. J. Mod. Phys. D18:1039,2009

Astronomy and Astrophysics

Astrophysics

Major revisions made; Matching the version to be published in IJMPD

Scientific paper

10.1142/S021827180901490X

In the framework of Relativistic MOND theory (TeVeS), we show that a late time background $\Lambda$CDM cosmology can be attained by choosing a specific $F(\mu)$ that also meets the requirement for the existence of Newtonian and MOND limits. We investigate the dynamics of the scalar field $\phi$ under our chosen $F(\mu)$ and show that the "slow roll" regime of $\phi$ corresponds to a dynamical attractor, where the whole system reduces to $\Lambda$CDM cosmology.

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