Radiative Contributions to Conservative Binary Dynamics - Stefano Foffa
Offered By: Kavli Institute for Theoretical Physics via YouTube
Course Description
Overview
Explore radiative contributions to conservative binary dynamics in this 40-minute lecture by Stefano Foffa from the University of Geneva. Delve into the impact of gravitational wave detection on various fields of physics, from field theory to cosmology. Examine the precision modeling required for interpreting gravitational-wave events and searching for new physics. Learn about the self-force limit, effective theory, and multipole results. Investigate the effective action, conservative and dissipative parts, and the absence of conserved energy. Analyze memory diagrams, dissipative contributions, and radiation to infinity. Understand the optical theorem's application to gravitational waves and fields. Gain insights into the challenges and recent advances in gravitational wave modeling, as well as emerging tools and techniques from classical and quantum field theory.
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
Related Courses
Extraordinary Physics with Millisecond Pulsars - Scott RansomInstitute for Advanced Study via YouTube The Extreme Instruments of Astrophysics - LIGO
Hackaday via YouTube Gravitational Wave Astronomy
Hubble Space Telescope via YouTube Gravitational Waveforms for Compact Binaries - Jan Steinhoff
Kavli Institute for Theoretical Physics via YouTube Millisecond Pulsars by Professor G Srinivasan
International Centre for Theoretical Sciences via YouTube