The self-gravitating gas in the presence of dark energy: Monte Carlo simulations and stability analysis

DOI10.1016/j.nuclphysb.2005.08.006zbMath1126.83316arXivastro-ph/0410147OpenAlexW1988044664MaRDI QIDQ876216

J. A. Siebert, H. J. De Vega

Publication date: 16 April 2007

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0410147

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (2)

Gravitational instabilities of isothermal spheres in the presence of a cosmological constant ⋮ PHASE TRANSITIONS IN SELF-GRAVITATING SYSTEMS

Cites Work

• Statistical mechanics of gravitating systems
• The self-gravitating gas in the presence of the cosmological constant
• Monte Carlo simulation in statistical physics. An introduction
• The cosmological constant and dark energy
• Statistical mechanics of the self-gravitating gas. I: Thermodynamic limit and phase diagrams
• Statistical mechanics of the self-gravitating gas. II: Local physical magnitudes and fractal structures
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