Accretion of a relativistic, collisionless kinetic gas into a Schwarzschild black hole

DOI10.1088/1361-6382/AA65FAzbMath1369.83006arXiv1611.02389OpenAlexW2549679843MaRDI QIDQ5351998

Olivier Sarbach, Paola Rioseco

Publication date: 31 August 2017

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

Full work available at URL: https://arxiv.org/abs/1611.02389

zbMATH Keywords

integrable Hamiltonian systemsSchwarzschild black holerelativistic kinetic theoryblack hole accretion

Mathematics Subject Classification ID

Black holes (83C57) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Hamiltonian systems on groups of diffeomorphisms and on manifolds of mappings and metrics (37K65) Research exposition (monographs, survey articles) pertaining to astronomy and astrophysics (85-02)

Related Items (8)

Revisiting timelike and null geodesics in the Schwarzschild spacetime: general expressions in terms of Weierstrass elliptic functions ⋮ An introduction to the relativistic kinetic theory on curved spacetimes ⋮ Decay estimates for the massless Vlasov equation on Schwarzschild spacetimes ⋮ Kinetic gases in static spherically symmetric modified dispersion relations ⋮ Phase space mixing in an external gravitational central potential ⋮ Gravito-thermal transports, Onsager reciprocal relation and gravitational Wiedemann-Franz law ⋮ Axisymmetric, stationary collisionless gas configurations surrounding Schwarzschild black holes ⋮ Axisymmetric, stationary collisionless gas clouds trapped in a Newtonian potential

This page was built for publication: Accretion of a relativistic, collisionless kinetic gas into a Schwarzschild black hole