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1
Introduction
2
Gravitational waves
3
Observations
4
Simulations
5
Observations so far
6
What can we do
7
Overview
8
Why are we interested
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How do we merge
10
Mass distribution
11
Mass gaps
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Basis Theorem
13
Normal Distribution
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Spectral Density
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O3B
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Spins
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Spin examples
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Current network
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Current timeline
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Conclusion
21
Questions
22
Summary
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General questions
24
Audience question
25
Ligo Virgo
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December 2020
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Whats going to be sent out
28
Predictions
29
Detections
Description:
Explore the current state and future prospects of gravitational-wave astronomy in this comprehensive lecture by Christopher Berry from the University of Glasgow. Delve into the groundbreaking detection of gravitational waves by Advanced LIGO/Virgo and its far-reaching implications across physics, from field theory to stellar evolution and cosmology. Gain insights into the precision modeling required for interpreting strong gravitational-wave events and searching for new physics. Learn about upcoming advancements in detector sensitivity, both ground-based and space-based, and the challenges they present for theoretical physicists. Discover the collaborative efforts between classical relativity, effective field theory, and scattering amplitudes experts to address these challenges. Examine the mass distribution of black holes, spin properties, and current observational networks. Understand the importance of the Normal Distribution, Spectral Density, and Basis Theorem in gravitational wave analysis. Conclude with an overview of future predictions, detections, and the exciting developments expected in the field of gravitational-wave astronomy. Read more

The Status of Gravitational-Wave Astronomy - Christopher Berry

Kavli Institute for Theoretical Physics
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