Modeling galactic halos with predominantly quintessential matter

DOI10.1007/s10773-011-0761-7zbMath1252.85008arXiv1101.2515OpenAlexW2088065259MaRDI QIDQ763296

D. Kharzeev

Publication date: 9 March 2012

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

Full work available at URL: https://arxiv.org/abs/1101.2515

zbMATH Keywords

dark mattergalactic halosquintessential matter

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (2)

Galactic rotation curves inspired by a noncommutative-geometry background ⋮ A new proposal for galactic dark matter: effect of \(f(T)\) gravity

Cites Work

• Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
• GLOBAL MONOPOLE, DARK MATTER AND SCALAR TENSOR THEORY
• Quintessence and black holes
• On the Masses of Nebulae and of Clusters of Nebulae

This page was built for publication: Modeling galactic halos with predominantly quintessential matter