On axisymmetric and stationary solutions of the self-gravitating Vlasov system
Artikel i vetenskaplig tidskrift, 2016

Axisymmetric and stationary solutions are constructed to the Einstein-Vlasov and Vlasov-Poisson systems. These solutions are constructed numerically, using finite element methods and a fixed-point iteration in which the total mass is fixed at each step. A variety of axisymmetric stationary solutions are exhibited, including solutions with toroidal, disk-like, spindle-like, and composite spatial density configurations, as are solutions with non-vanishing net angular momentum. In the case of toroidal solutions, we show for the first time, solutions of the Einstein-Vlasov system which contain ergoregions.

matter

existence

spacetimes

relativistic stellar-systems

stability

Einstein-Vlasov

general-relativity

Vlasov-Poisson

rotation

spindle singularities

ergoregion

models

axisymmetric stationary solutions

Physics

galaxies

Astronomy & Astrophysics

Författare

Ellery Ames

Göteborgs universitet

Chalmers, Matematiska vetenskaper, Matematik

Håkan Andreasson

Chalmers, Matematiska vetenskaper, Matematik

Göteborgs universitet

Anders Logg

Chalmers, Matematiska vetenskaper, Matematik

Göteborgs universitet

Classical and Quantum Gravity

0264-9381 (ISSN)

Vol. 33 15 no. 155008- 155008

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.1088/0264-9381/33/15/155008

Mer information

Senast uppdaterat

2022-04-05