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- W2055145318 abstract "We extensively develop a perturbation theory for nonlinear cosmological dynamics, based on the Lagrangian description of hydrodynamics. We solve the hydrodynamic equations for a self-gravitating fluid with pressure, given by a polytropic equation of state, using a perturbation method up to second order. This perturbative approach is an extension of the usual Lagrangian perturbation theory for a pressureless fluid, in view of the inclusion of the pressure effect, which should be taken into account on the occurrence of velocity dispersion. We obtain the first-order solutions in generic background universes and the second-order solutions in a wider range of a polytropic index, whereas our previous work gives the first-order solutions only in the Einstein--de Sitter background and the second-order solutions for the polytropic index $4/3.$ Using the perturbation solutions, we present illustrative examples of our formulation in one- and two-dimensional systems, and discuss how the evolution of inhomogeneities changes for the variation of the polytropic index." @default.
- W2055145318 created "2016-06-24" @default.
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- W2055145318 date "2002-09-25" @default.
- W2055145318 modified "2023-09-27" @default.
- W2055145318 title "Perturbation theory in Lagrangian hydrodynamics for a cosmological fluid with velocity dispersion" @default.
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- W2055145318 doi "https://doi.org/10.1103/physrevd.66.064014" @default.
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