Overview
Explore groundbreaking research in a CITA presentation examining how the Galactic bar's resonant dynamics can be used to probe dark matter. Delve into complex topics including inertial mass, angle action variables, and the Bus Spindown phenomenon while learning about stars near the Sun and the history of the Hyperstream. Follow along as speaker Rimpei Chiba presents test particle simulation results, theoretical explanations, and detailed analysis of bar resonance and radial actions. Gain insights into the relationship between metallicity, resonance evolution, and slowing rates in this comprehensive examination of galactic dynamics and dark matter detection methods.
Syllabus
Introduction
Motivation
Inertial mass
Angle action variables
Bus Spindown
Stars near the Sun
History of the Hyperstream
Test Particle Simulation
Comparing the results
Theoretical explanation
Slowing rate
Metallicity
Resonance evolution
Bar resonance
Radial actions
Analysis
Discussion
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