Galactic cluster in the presence of Dark Energy

DOI10.1134/S0202289314030049zbMath1308.85004arXiv1303.7166OpenAlexW2079129139MaRDI QIDQ2018677

Gennady S. Bisnovatyi-Kogan

Publication date: 25 March 2015

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1303.7166

zbMATH Keywords

cosmological constantdark matterpolytropic gascosmic rayscosmological expansionhydrodynamic outflow

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Stability and instability of geophysical and astrophysical flows (76E20) Radiative transfer in astronomy and astrophysics (85A25) Astrophysical cosmology (85A40)

Cites Work

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• Dark energy and key physical parameters of clusters of galaxies
• Cosmological parameters from SDSS and WMAP
• A brief analysis of self-gravitating polytropic models with a non-zero cosmological constant
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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