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Phase space mixing of a Vlasov gas in the exterior of a Kerr black hole

GGD - Gr@V Seminar
Speaker
Olivier Sarbach (Universidad Autónoma Metropolitana Cuajimalpa, Universidad Michoacana de San Nicolás de Hidalgo)
Event date
Venue
On-site: Sala Sousa Pinto
Event Website
Event type

We analyze the dynamics of a collisionless kinetic gas propagating in the exterior of a rotating Kerr black hole. We focus on the phase space region corresponding to orbits that are bounded in space.

12 million CPU-hours awarded to our group

A computing proposal prepared by S. Gimeno-Soler, P. Cunha, I. Sengo and C. Herdeiro, and led by H. Olivares was awarded with 12 million CPU-hours at the supercomputer Mare Nostrum 5.
The project, titled "Exploring accretion and spacetime models for event-horizon-scale observations of low-luminosity active galactic nuclei", will explore new models of accretion flows and spacetime geometries for the targets of the Event Horizon Telescope using simulations as the one shown in the picture (Image credit: H. Olivares and P. Cunha).