Speaker
Fupeng Zhang
Description
Recently we have build a Monte-Carlo method that can obtain self-consistent solutions of an evolving nuclear star cluster that contains a central massive black hole. Our method evolves the orbits of stellar objects by solving two-dimensional (energy and angular momentum) Fokker-Planck equations given multiple mass components. In this study we apply our method to investigate the evolution of the rates of extreme mass ratio inspirals over cosmic time.
Primary author
Co-author
Prof.
Pau Amaro Seoane
(Universitat Politècnica de València, Spain)
