Simulating Accretion in the Inner Cavity of Circumbinary Disks - Philipp Moesta
Kavli Institute for Theoretical Physics via YouTube
Overview
Explore a conference talk on simulating accretion in the inner cavity of circumbinary disks, presented by Philipp Moesta from the University of Amsterdam. Delve into the complexities of binary systems, from stars to supermassive black holes, and their interactions with surrounding circumbinary gas. Learn about the evolution of this gas, its influence on embedded binaries, and the observational signatures that provide valuable insights. Discover the novel numerical techniques required to model these systems effectively. Gain perspective on the similarities between massive black hole binaries and stellar binaries, and understand the importance of bringing together these two distinct research communities. Examine topics such as project setup, modelling eccentricity, orbital evolution, internal cavity characteristics, potential shock emission, and microphysics. Engage with the latest advancements in observations of stellar binaries and numerical modeling of both stars and black holes, while considering the crucial next steps in expanding our knowledge of these fascinating astrophysical phenomena.
Syllabus
Introduction
How did you set up the project
What did you like about the project
Modelling eccentricity
Evolution during one orbit
How can we quantify
Internal cavity size
Internal cavity area
Potential shock emission
Microphysics
Summary
Questions
Discussion
Taught by
Kavli Institute for Theoretical Physics