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Mordehai Milgrom
Particle Dark Matter an Introduction Into Evidence, Models, and Direct Searches
X-Ray Shapes of Elliptical Galaxies and Implications for Self-Interacting Dark Matter
Explosion of the Science Modification of Newtonian Dynamics Via Mach's
Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions Benoit Famaey, Stacy S
What Is Real?
Arxiv:Astro-Ph/0701848V1 30 Jan 2007 Xetd Tesaclrto Eas Ti H Quantity the Is It Because Than Acceleration Bigger Stress Much I Are Velocities Expected
The Board of Governors
Lagrangian Formulation of Mond; Mond Field in Perturbed Spherical Systems
MOND Vs. Dark Matter in Light of Historical Parallels
Toomre Stability of Disk Galaxies in Quasi-Linear MOND
Epistemology of Experimental Gravity - Scientific Rationality
A Matter of Universal Interest
Modified Einsteinian Dynamics
MOND Also Lurks out There—The Infamous Dark Matter
Mond — Particularly As Modified Inertia∗
MOND As a Regime of Quantum Gravity Arxiv:1704.00780V2 [Gr-Qc]
UNIVERSITY of CALIFORNIA SANTA CRUZ MULTI-WAVELENGTH ASTROPHYSICAL PROBES of DARK MATTER PROPERTIES a Dissertation Submitted In
THE MODIFIED NEWTONIAN DYNAMICS AS an ALTERNATIVE to HIDDEN MATTER Mordehai Milgrom * Canadian Institute for Theoretical Astroph
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