Galaxies with Fuzzy Dark Matter

Abstract

This is a brief review on some properties of galaxies in the fuzzy dark matter model, where dark matter is an ultra-light scalar particle with mass $m=O(10^{-22})eV$. From quantum pressure, dark matter has a halo length scale which can solve the small scale issues of the cold dark matter model, such as the core-cusp problem, and explain many other observed mysteries of galaxies.

References in corpus (8)

• Big-Bang Nucleosynthesis
• Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
• The Radial Acceleration Relation in Rotationally Supported Galaxies
• Understanding the Core-Halo Relation of Quantum Wave Dark Matter, $\psi$DM, from 3D Simulations
• A common mass scale for satellite galaxies of the Milky Way
• Bose-Einstein Condensation of Dark Matter Axions
• Are galaxies extending?
• Radial Acceleration Relation from Ultra-light Scalar Dark matter