The self-gravitating gas in the presence of the cosmological constant

DOI10.1016/j.nuclphysb.2004.11.013zbMath1160.83365arXivastro-ph/0305322OpenAlexW70159914MaRDI QIDQ874609

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

Publication date: 10 April 2007

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

Full work available at URL: https://arxiv.org/abs/astro-ph/0305322

zbMATH Keywords

cosmological constantmean field theoryhydrostatics of the self-gravitating gasNon-relativistic gravitypartition function of the self-gravitating gasspherically symmetric case

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (4)

Comment on: ``The cluster expansion for the self-gravitating gas and the thermodynamic limit by de Vega and Sanchez ⋮ The self-gravitating gas in the presence of dark energy: Monte Carlo simulations and stability analysis ⋮ Gravitational instabilities of isothermal spheres in the presence of a cosmological constant ⋮ PHASE TRANSITIONS IN SELF-GRAVITATING SYSTEMS

Cites Work

• 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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