Optimal transport by omni-potential flow and cosmological reconstruction

DOI10.1063/1.3691203zbMath1274.83151arXiv1111.2516OpenAlexW3101117373MaRDI QIDQ2861751

Vladislav Zheligovsky, Barbara Villone, Olga M. Podvigina, Uriel Frisch

Publication date: 11 November 2013

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1111.2516

zbMATH Keywords

WKB techniqueZeldovich flows

Mathematics Subject Classification ID

PDEs in connection with fluid mechanics (35Q35) Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (2)

Causality for nonlocal phenomena ⋮ Generally covariant \(N\)-particle dynamics

Cites Work

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• The reconstruction problem for the Euler-Poisson system in cosmology
• Auction algorithms for network flow problems: A tutorial introduction
• Large-scale structure of the universe and cosmological perturbation theory
• Notes on the three-dimensional flow pattern of a perfect fluid in the presence of a small perturbation of the initial velocity field
• Polar factorization and monotone rearrangement of vector‐valued functions
• Optimal Transport

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