Rotational velocity curves in the Milky Way as a test of modified gravity

J. W. Moffat and V. T. Toth
Phys. Rev. D 91, 043004 – Published 17 February 2015

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 is in excellent agreement with data for the Milky Way without a dark matter halo, with a mass of 5×1010M. The velocity rotation curve predicted by modified Newtonian dynamics does not agree with the data.

  • Figure
  • Received 24 December 2014

DOI:https://doi.org/10.1103/PhysRevD.91.043004

© 2015 American Physical Society

Authors & Affiliations

J. W. Moffat1,2 and V. T. Toth1

  • 1Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada
  • 2Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 91, Iss. 4 — 15 February 2015

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×