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This talk examines observational evidence for dark matter, including galaxy clusters, galactic rotation curves, gravitational lensing, the cosmic microwave background, and structure formation. It also considers modified gravity and superfluid dark matter as alternative explanations and discusses possible tests.
Syllabus
Intro
trophysicists introduce new "stuff" to fix the problem
What is Dark Matter?
Galaxy Clusters
Galactic Rotation Curves
Gravitational Lensing
The Cosmic Microwave Background
Structure Formation
How Dark Matter solves the problem
Can Dark Matter be "normal" matter?
Alternative Explanation: Modified Gravity
How does Modified Newtonian Dynamics work?
Dark Matter, Pimped
What is a Superfluid?
SFDM fits the Milky Way Rotation Curve nicely
Ways to test superfluid dark matter
Summary
Taught by
The Royal Institution