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Radiative Contributions to Conservative Binary Dynamics - Stefano Foffa

Kavli Institute for Theoretical Physics via YouTube

Overview

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This course aims to explore the radiative contributions to conservative binary dynamics in the context of gravitational wave detection. The learning outcomes include understanding the impact of gravitational wave signals on various areas of physics, interpreting gravitational wave events, and identifying new physics embedded in these signals. The course teaches skills such as precision modeling of gravitational wave signals, discussing the needs of future experiments, and highlighting recent advances in gravitational wave modeling. 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 physics and theoretical physics.

Syllabus

Introduction
Selfforce limit
Effective theory
Noncontroversial
Multiples
Results
Problems
Effective action
Conclusions
Conservative dissipative parts
No conserved energy
G204s
Memory diagrams
Dissipative contributions
Diagrams
Radiation to infinity
Optical theorem
Gravitational waves
Gravitational fields
My confusion

Taught by

Kavli Institute for Theoretical Physics

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