Rotational Velocity Curves in the Milky Way as a Test of Modified Gravity
J. W. Moffat, V. T. Toth

TL;DR
This paper tests modified gravity theories using the Milky Way's rotation curve, finding Scalar-Vector-Tensor Gravity matches observations without dark matter, unlike MOND.
Contribution
It demonstrates that Scalar-Vector-Tensor Gravity accurately predicts the Milky Way's rotation curve without dark matter, challenging MOND's predictions.
Findings
STVG/MOG matches observed rotation curves
MOND's predictions do not align with data
Supports modified gravity as an alternative to dark matter
Abstract
Galaxy rotation curves determined observationally out to a radius well beyond the galaxy cores can provide a critical test of modified gravity models without dark matter. The predicted rotational velocity curve obtained from Scalar-Vector-Tensor Gravity (STVG or MOG) is in excellent agreement with data for the Milky Way without a dark matter halo, with a mass of . The velocity rotation curve predicted by modified Newtonian Dynamics (MOND) does not agree with the data.
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