Modified Newtonian Dynamics of Large Scale Structure

Details Modified Newtonian Dynamics of Large Scale Structure Modified Newtonian Dynamics of Large Scale Structure

2001-09-03

arxiv.org/abs/astro-ph/0109016v2

Mon.Not.Roy.Astron.Soc. 331 (2002) 909

Astronomy and Astrophysics

Astrophysics

Version accepted for publication in the MNRAS. Results of more simulations are included

Scientific paper

10.1046/j.1365-8711.2002.05235.x

We examine the implications of Modified Newtonian Dynamics (MOND) on the large scale structure in a Friedmann-Robertson-Walker universe. We employ a ``Jeans swindle'' to write a MOND-type relationship between the fluctuations in the density and the gravitational force, $\vg$. In linear Newtonian theory, $|\vg|$ decreases with time and eventually becomes $

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