Michel accretion of a polytropic fluid with adiabatic index $\gamma \gt 5/3$: global flows versus homoclinic orbits

DOI10.1088/0264-9381/33/10/105016zbMath1338.83102arXiv1511.07728OpenAlexW3124960202MaRDI QIDQ2811475

Patryk Mach, Eliana Chaverra, Olivier Sarbach

Publication date: 10 June 2016

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1511.07728

zbMATH Keywords

black holesSchwarzschildHamiltonian dynamical systemsaccretion flows

Mathematics Subject Classification ID

Black holes (83C57) Dynamical systems in other branches of physics (quantum mechanics, general relativity, laser physics) (37N20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Hamilton-Jacobi equations in mechanics (70H20)

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Dissipation and acoustic tunnelling about the sonic horizon of Bondi accretion ⋮ Matter accretion onto higher-dimensional black holes with Dirac-Born-Infeld global defects via well known fluids ⋮ Relativistic low angular momentum accretion: long time evolution of hydrodynamical inviscid flows

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