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Wave Dark Matter Production - Lecture II

Galileo Galilei Institute (GGI) via YouTube

Overview

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Explore the theoretical foundations and production mechanisms of wave dark matter in this comprehensive physics lecture that delves into advanced concepts of cosmological dark matter candidates. Learn about the wave-like properties of dark matter particles, including axions and other ultralight bosons, and examine how these particles are produced in the early universe through various mechanisms such as vacuum misalignment, topological defects, and parametric resonance. Discover the mathematical frameworks used to describe wave dark matter dynamics, including the Schrödinger-Poisson equation and its applications to structure formation. Analyze the observational signatures and detection strategies for wave dark matter, covering topics such as interference patterns, coherence lengths, and the distinctive features that differentiate wave dark matter from traditional cold dark matter models. Investigate current theoretical challenges and recent developments in the field, including the role of self-interactions, quantum pressure effects, and the formation of solitonic cores in dark matter halos.

Syllabus

Marco Gorghetto: "Wave Dark Matter production"- Lecture II

Taught by

Galileo Galilei Institute (GGI)

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