Kinetic Gas Disks Surrounding Schwarzschild Black Holes
نویسندگان
چکیده
We describe stationary and axisymmetric gas configurations surrounding black holes. They consist of a collisionless relativistic kinetic identical massive particles following bound orbits in Schwarzschild exterior spacetime are modeled by one-particle distribution function which is the product energy orbital inclination associated with particle's trajectory. The morphology resulting configuration analyzed.
منابع مشابه
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ژورنال
عنوان ژورنال: Acta Physica Polonica
سال: 2022
ISSN: ['2082-7865', '1899-2358']
DOI: https://doi.org/10.5506/aphyspolbsupp.15.1-a10