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arXiv · 2202.00209

Kinetic gas disks surrounding Schwarzschild black holes

Carlos Gabarrete·Olivier Sarbach
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Abstract

We describe stationary and axisymmetric gas configurations surrounding black holes. They consist of a collisionless relativistic kinetic gas of identical massive particles following bound orbits in a Schwarzschild exterior spacetime and are modeled by a one-particle distribution function which is the product of a function of the energy and a function of the orbital inclination associated with the particle's trajectory. The morphology of the resulting configuration is analyzed.

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Carlos Gabarrete, Olivier Sarbach. 2022-02-01. Kinetic gas disks surrounding Schwarzschild black holes. https://doi.org/10.5506/aphyspolbsupp.15.1-a10

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