This course explores the concept of compact binary mergers as multimessenger sources of gravitational waves. The learning outcomes include understanding the generation of gravitational waves from compact binaries and the potential for observable electromagnetic and neutrino counterparts. The course covers skills such as interpreting magnetohydrodynamic simulations in general relativity and discussing the launch of jets from black hole-neutron star mergers. The teaching method includes lectures, simulations, and showcasing computer-generated movies. The intended audience for this course is individuals interested in astrophysics, gravitational waves, and multimessenger astronomy.
Overview
Syllabus
Introduction
Overview
Gravitational Waves
First Binary Pulsar
Gravitational Wave Detection
Pulsar Timing Array
Laser Interferometer
Lisa Pathfinder
Compact Binary Mergers
Multimessenger Sources
Which Detector to Use
How to Measure the Wave
Short GammaRay Burst Source
GammaRay Burst Source
Illinois GMHD Code
Simulation Summary
Catalina Survey
PanSTARRS
Group 1 Simulation
Conclusion
Questions
Conclusions
Taught by
APS Physics
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