The dark matter distribution function and halo thermalization from the Eddington equation in galaxies

DOI10.1142/S0217751X16500731zbMath1338.85004arXiv1401.0726OpenAlexW3100445431MaRDI QIDQ2812744

N. G. Sánchez, H. J. De Vega

Publication date: 13 June 2016

Published in: International Journal of Modern Physics A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1401.0726

zbMATH Keywords

dark mattergalaxy structuregalaxy density profiles

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Observational and experimental questions in relativity and gravitational theory (83B05) Galactic and stellar structure (85A15) Astrophysical cosmology (85A40)

Related Items (1)

Estimation of the mass of dark matter using the observed mass profiles of late-type galaxies

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