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Nonlinear theory of the development of potential perturbations
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inferredcites →https://doi.org/10.3367/ufnr.0080.196307d.0391openalex-snapshot
Problems of relativistic cosmology
What points at this work
Incoming claims: where this work appears in other papers’ reference lists and arguments.
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Evolution of Potential Perturbations after Decoupling (The Adiabatic Scenario)
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The large scale structure of the universe I. General properties. One-and two-dimensional models
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Evolution of the Power Spectrum and Self‐Similarity in the Expanding One‐dimensional Universe
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Universality in the Distribution of Caustics in the Expanding Universe
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Lagrangian perturbations and the matter bispectrum I: fourth-order model for non-linear clustering
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Lagrangian volume deformations around simulated galaxies
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Post-collapse perturbation theory in 1D cosmology – beyond shell-crossing
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Beyond relativistic Lagrangian perturbation theory: An exact-solution controlled model for structure formation
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Nonperturbative collapse models for collisionless self-gravitating flows
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Back reaction of inhomogeneities on the expansion: The evolution of cosmological parameters
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Large-scale structure of the Universe. The Zeldovich approximation and the adhesion model
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On General-Relativistic Lagrangian Perturbation Theory and Its Non-Perturbative Generalization
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Inhomogeneous Relativistic Cosmology : nonperturbative models and spatial averaging of the Einstein equations
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Modélisation Bayésienne des mesures de vitesses particulières dans le projet CosmicFlows
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