Description of the evolution of inhomogeneities on a dark matter halo with the Vlasov equation

DOI10.1007/S10714-017-2286-8zbMath1380.85005arXiv1703.03286OpenAlexW2600469039MaRDI QIDQ1697889

Erik Jiménez-Vázquez, Paola Domínguez-Fernández, Darío Núñez, Miguel Alcubierre, Edison Montoya

Publication date: 20 February 2018

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1703.03286

zbMATH Keywords

numerical methodscosmologydark matterVlasov equationhaloevolution of inhomogeneities

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

Related Items (3)

Phase space mixing in an external gravitational central potential ⋮ Phase mixing for solutions to 1D transport equation in a confining potential ⋮ Axisymmetric, stationary collisionless gas clouds trapped in a Newtonian potential

Cites Work

• Scalar fields as dark matter in spiral galaxies
• Scalar field as dark matter in the universe
• The Einstein-Vlasov system/kinetic theory
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