24 July 2023 to 4 August 2023
Warszawa/Chęciny
Europe/Warsaw timezone

Session

Particle motion and dynamics of a Vlasov gas in the exterior of a Kerr black hole

31 Jul 2023, 09:00

Conveners

Particle motion and dynamics of a Vlasov gas in the exterior of a Kerr black hole

  • Olivier Sarbach (Universidad Michoacana de San Nicolás de Hidalgo)

Particle motion and dynamics of a Vlasov gas in the exterior of a Kerr black hole

  • Olivier Sarbach (Universidad Michoacana de San Nicolás de Hidalgo)

Particle motion and dynamics of a Vlasov gas in the exterior of a Kerr black hole

  • Olivier Sarbach (Universidad Michoacana de San Nicolás de Hidalgo)

Particle motion and dynamics of a Vlasov gas in the exterior of a Kerr black hole

  • Olivier Sarbach (Universidad Michoacana de San Nicolás de Hidalgo)

Particle motion and dynamics of a Vlasov gas in the exterior of a Kerr black hole

  • Olivier Sarbach (Universidad Michoacana de San Nicolás de Hidalgo)

Description

These lectures start with a discussion of some of the properties of the most important black hole solution in general relativity and relativistic astrophysics: the Kerr black hole. In particular, the notions of static and stationary observers, ergospheres, horizons, causal structure and the motion of free-falling massive and massless particles will be reviewed. Next, some tools are introduced to understand the geometry of the cotangent bundle associated with a (generic) curved spacetime (M,g). Based on these tools, a manifestly covariant theory is derived describing a relativistic Vlasov gas, that is, a gas consisting of collisionless particles propagating in (M,g). In the final part of the lectures, this theory is applied to the study of the dynamics of a Vlasov gas consisting of particles which follow spatially bound timelike geodesics in the exterior of a Kerr black hole. To this purpose, generalized action-angle variables are introduced in which the geodesic flow simplify considerably and the relativistic Vlasov equation can be solved analytically. Based on this representation, it is shown that - even though it is collisionless - the gas undergoes a relaxation process and settles down to a stationary, axisymmetric configuration. The underlying mechanism for this effect, which is due to phase mixing, will be explained.

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