Mass power spectrum in a universe dominated by the Chaplygin gas

DOI10.1023/A:1021187518781zbMath1015.83016arXivastro-ph/0203441OpenAlexW3099026380MaRDI QIDQ1863122

P. E. de Souza, Sergio Vitorino B. Gonçalves, Júlio César Fabris

Publication date: 11 March 2003

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0203441

zbMATH Keywords

perturbationspectrumChaplygin gasuniverse modelperturbation spectrumpure baryonic universe

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items

Can the cosmological dark sector be modeled by a single scalar field? ⋮ Thermodynamics of modified cosmic Chaplygin gas ⋮ Statefinder diagnostic for modified Chaplygin gas cosmology in f(R,T) gravity with particle creation ⋮ Schrödinger-Wheeler-DeWitt equation in Chaplygin gas FRW cosmological model ⋮ Chaplygin gas quantum universe in the presence of the cosmological constant ⋮ Instability of holographic dark energy models ⋮ OBSERVATIONAL CONSTRAINTS ON THE GENERALIZED CHAPLYGIN GAS ⋮ Attractor inflationary solutions in braneworld scenario

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