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Overview
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Explore how machine learning techniques can be applied to map the distribution of dark matter in our local cosmic neighborhood in this hour-long conference presentation. Learn about cutting-edge computational methods and algorithms used to analyze astronomical data and infer the presence and distribution of dark matter, which makes up approximately 85% of all matter in the universe but cannot be directly observed. Discover the challenges astronomers face when studying dark matter's gravitational effects on visible matter and how advanced machine learning models help overcome observational limitations. Examine specific case studies and research findings that demonstrate how these techniques reveal dark matter's role in galaxy formation and cosmic structure evolution. Gain insights into the intersection of astrophysics, cosmology, and artificial intelligence as researchers work to understand one of the universe's most mysterious components through innovative data analysis approaches.
Syllabus
1130: Mapping the Local Dark Matter Distribution through Machine Learning
Taught by
CITA Presentations