Variable Modified Newtonian Mechanics III: Milky Way Rotational Curve
James C. C. Wong

TL;DR
This paper proposes a modified Newtonian mechanics model, VMOND, incorporating cosmological background effects, to explain the Milky Way's rotational curve, matching Gaia observations without dark matter.
Contribution
It introduces a new cosmological background-dependent MOND-like acceleration model and applies it to galaxy formation, successfully reproducing observed rotation curves.
Findings
Model reproduces Milky Way rotation curve closely.
Predicts a radius-dependent acceleration similar to MOND.
Establishes a Baryonic Tully-Fisher Relation from the model.
Abstract
For a point mass residing in an expanding universe, within General Relativity (GR), a new metric [1} is found to lead to a cosmological background dependent MOND-like acceleration in addition to the Newtonian acceleration. In [2], we study the monolithic evolution of a spherical overdensity at recombination in this combined acceleration, called VMOND. Under reasonable relaxation assumptions we find that a massive spherical galaxy with a stable core can from at . For galaxy mass and a realistic initial overdensity, the model late time MOND acceleration at radius r takes on values similar to the canonical MOND acceleration at large radius r. In this work, we consider an idealised model of rotating galaxy formation in which a Milky Way mass overdensity under VMOND monolithically evolves into a virialised sphere. We assume that this…
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Taxonomy
TopicsCosmology and Gravitation Theories · Radio Astronomy Observations and Technology · Relativity and Gravitational Theory
