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arxiv: 1108.5588 · v2 · pith:JYEWCU34new · submitted 2011-08-29 · 🌌 astro-ph.CO · astro-ph.GA· gr-qc

Recovering MOND from extended metric theories of gravity

classification 🌌 astro-ph.CO astro-ph.GAgr-qc
keywords gravitylimitmondtheoryweak-fieldapproachextendedmetric
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We show that the Modified Newtonian Dynamics (MOND) regime can be fully recovered as the weak-field limit of a particular theory of gravity formulated in the metric approach. This is possible when Milgrom's acceleration constant is taken as a fundamental quantity which couples to the theory in a very consistent manner. As a consequence, the scale invariance of the gravitational interaction is naturally broken. In this sense, Newtonian gravity is the weak-field limit of general relativity and MOND is the weak-field limit of that particular extended theory of gravity. We also prove that a Noether's symmetry approach to the problem yields a conserved quantity coherent with this relativistic MONDian extension.

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  1. Baryonic mass budgets in the central regions of the Bullet Cluster and their consistency with strong lensing in MOND

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    IGIMF-based baryonic mass estimates for three Bullet Cluster BCG cores using JWST photometry place the MOND strong-lensing masses inside the predicted baryonic range.