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Accretion of the relativistic Vlasov gas onto a moving Schwarzschild black hole: Low-temperature limit and numerical aspects

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arxiv 2202.02173 v1 pith:6LJZCNM3 submitted 2022-02-04 gr-qc

Patryk Mach , Andrzej Odrzywolek This is my paper · ORCID
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keywords accretionlimitaspectsblackdensityholelow-temperaturemoving
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New developments related to our recent study of the accretion of the Vlasov gas onto a moving Schwarzschild black hole are presented. We discuss the low-temperature limit of the mas accretion rate and a simple Monte Carlo simulation used to check the results obtained in this limit. We also comment on several numerical aspects related with momentum integrals expressing the particle density current and the particle density.

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  1. A discussion on the symmetry of relativistic Vlasov gas and its accretion in Kerr-Newman black hole

    gr-qc 2025-06 conditional novelty 4.0 of 10

    For Kerr-Newman black holes, the Vlasov gas distribution depends only on constants of motion, and computed accretion rates push the hole toward Schwarzschild.

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