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A dynamic model of spherical perturbations in the Friedmann universe. III. Self-similar solutions - MaRDI portal

A dynamic model of spherical perturbations in the Friedmann universe. III. Self-similar solutions (Q1033697)

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A dynamic model of spherical perturbations in the Friedmann universe. III. Self-similar solutions
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    A dynamic model of spherical perturbations in the Friedmann universe. III. Self-similar solutions (English)
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    10 November 2009
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    gravitation theory
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    cosmology
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    spherical perturbation theory
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    boundary value problem
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