The need for dark matter in galaxies

Abstract

Cooperstock and Tieu have proposed a model to account for galactic rotation curves without invoking dark matter. I argue that no model of this type can work.

References in corpus (1)

• Post-Newtonian Gravitational Radiation and Equations of Motion via Direct Integration of the Relaxed Einstein Equations. I. Foundations

Cited by in corpus (9)

• Non-Newtonian behavior in weak field general relativity for extended rotating sources
• Galactic Dynamics via General Relativity: A Compilation and New Developments
• Anisotropic Models for Globular Clusters, Galactic Bulges and Dark Halos
• Kinetic Theory of Collisionless Self-Gravitating Gases: II. Relativistic Corrections in Galactic Dynamics
• Why do we Still Believe in Newton's Law ? Facts, Myths and Methods in Gravitational Physics
• A darkless space-time
• General Relativistic Thick Disks in the Accelerating Expanding Universe Dominated By Dark Energy
• Does Smoothing Matter?
• Immanuel Kant on Supersymmetry: A Practical Evaluation