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The Status of Gravitational-Wave Astronomy - Christopher Berry

Kavli Institute for Theoretical Physics via YouTube

Overview

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This course focuses on the status of gravitational-wave astronomy, exploring the impact of gravitational wave detection on various areas of physics. The learning outcomes include understanding the needs of future gravitational-wave experiments, identifying theoretical challenges, discussing recent advances in gravitational wave modeling, and uncovering tools and techniques from classical and quantum field theory. The course teaches skills such as precision modeling of gravitational-wave signals, interpreting gravitational-wave events, and enabling searches for new physics embedded in these signals. The teaching method involves expert discussions from classical relativity, effective field theory, and scattering amplitudes communities. The intended audience includes researchers, scholars, and professionals interested in gravitational-wave astronomy, theoretical physics, and field theory.

Syllabus

Introduction
Gravitational waves
Observations
Simulations
Observations so far
What can we do
Overview
Why are we interested
How do we merge
Mass distribution
Mass gaps
Basis Theorem
Normal Distribution
Spectral Density
O3B
Spins
Spin examples
Current network
Current timeline
Conclusion
Questions
Summary
General questions
Audience question
Ligo Virgo
December 2020
Whats going to be sent out
Predictions
Detections

Taught by

Kavli Institute for Theoretical Physics

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