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Related papers: Caustic Skeleton & Cosmic Web

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The cosmic web is a complex spatial pattern of walls, filaments, cluster nodes and underdense void regions. It emerged through gravitational amplification from the Gaussian primordial density field. Here we infer analytical expressions for…

Cosmology and Nongalactic Astrophysics · Physics 2014-12-17 Job Feldbrugge , Johan Hidding , Rien van de Weygaert

We describe how the dynamics of cosmic structure formation defines the intricate geometric structure of the spine of the cosmic web. The Zeldovich approximation is used to model the backbone of the cosmic web in terms of its singularity…

Cosmology and Nongalactic Astrophysics · Physics 2013-11-28 Johan Hidding , Sergei F. Shandarin , Rien van de Weygaert

The cosmic web consists of a complex configuration of voids, walls, filaments, and clusters, which formed under the gravitational collapse of Gaussian fluctuations. Understanding under what conditions these different structures emerge from…

Cosmology and Nongalactic Astrophysics · Physics 2023-03-08 Job Feldbrugge , Rien van de Weygaert

Cosmic filaments are the main transport channels of matter in the Megaparsec universe, and represent the most prominent structural feature in the matter and galaxy distribution. Here we describe and define the physical and dynamical nature…

Cosmology and Nongalactic Astrophysics · Physics 2024-06-03 Job Feldbrugge , Rien van de Weygaert

The caustic skeleton is a parameter-free and mathematically rigorous formalism for tracing the hierarchical formation history of the multiscale cosmic web from the singularities in the underlying dark matter flow. In the present study, we…

Cosmology and Nongalactic Astrophysics · Physics 2026-04-21 Benjamin Hertzsch , Job Feldbrugge , Rien van de Weygaert

The caustic skeleton model is a mathematically rigorous framework for studying the formation history of the emerging cosmic web from the caustics in the underlying dark matter flow. In a series of two papers, we use constrained N-body…

Cosmology and Nongalactic Astrophysics · Physics 2025-10-06 Benjamin Hertzsch , Job Feldbrugge , Maé Rodriguez , Rien van de Weygaert

In 1970 Zel'dovich published a far-reaching paper presenting a simple equation describing the nonlinear growth of primordial density inhomogeneities. The equation was remarkably successful in explaining the large scale structure in the…

Cosmology and Nongalactic Astrophysics · Physics 2016-11-15 Bernard J. T. Jones , Rien van de Weygaert

We investigate the nonlinear evolution of cosmic morphologies of the large-scale structure by examining the Lagrangian dynamics of various tensors of a cosmic fluid element, including the velocity gradient tensor, the Hessian matrix of the…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-18 Xin Wang , Alex Szalay

Matter density is formally infinite at the location of caustic surfaces, where dark matter sheet folds in phase-space. The caustics separate regions with different number of streams and the volume elements change the parity by turning…

Cosmology and Nongalactic Astrophysics · Physics 2019-06-17 Sergei F. Shandarin , Nesar S. Ramachandra

I review the nature of three-dimensional collapse in the Zeldovich approximation, how it relates to the underlying nature of the three-dimensional Lagrangian manifold and naturally gives rise to a hierarchical structure formation scenario…

Cosmology and Nongalactic Astrophysics · Physics 2016-10-20 Oliver Hahn

Caustics-envelopes formed by the trajectories of fluid particles-arise in proposed dynamical extensions for shell-crossing singularities occurring in the Einstein-dust system. In this study, a local existence result is established,…

General Relativity and Quantum Cosmology · Physics 2025-12-09 David Bick

The local theory of the critical lines of 2D and 3D Gaussian fields that underline the cosmic structures is presented. In the context of cosmological matter distribution the subset of critical lines of the 3D density field serves to…

Astrophysics · Physics 2015-05-13 D. Pogosyan , C. Pichon , C. Gay , S. Prunet , J. F. Cardoso , T. Sousbie , S. Colombi

The Lagrangian theory of structure formation in cosmological fluids, restricted to the matter model ``dust'', provides successful models of large-scale structure in the Universe in the laminar regime, i.e., where the fluid flow is…

Astrophysics · Physics 2011-05-23 Susanne Adler , Thomas Buchert

We study the statistical properties of the eigenvalues of the primordial tidal and deformation tensor for random Gaussian cosmic density fields. With the tidal and deformation tensors, Hessians of the gravitational and velocity potential,…

Cosmology and Nongalactic Astrophysics · Physics 2023-01-19 Job Feldbrugge , Yihan Yan , Rien van de Weygaert

The cosmic large scale structure encodes the formation and evolution of a weblike network of dark matter and galaxies within the Universe. The cosmological information is wrapped up in non-Gaussian statistics requiring characterisation…

Cosmology and Nongalactic Astrophysics · Physics 2024-11-26 Alex Gough

A method to compute the full hierarchy of the critical subsets of a density field is presented. It is based on a watershed technique and uses a probability propagation scheme to improve the quality of the segmentation by circumventing the…

Astrophysics · Physics 2009-11-13 T. Sousbie , S. Colombi , C. Pichon

The cosmic web defines the large scale distribution of matter we see in the Universe today. Classifying the cosmic web into voids, sheets, filaments and nodes allows one to explore structure formation and the role environmental factors have…

Cosmology and Nongalactic Astrophysics · Physics 2016-02-24 J. D. Fisher , A. Faltenbacher , M. S. T. Johnson

A dynamical classification of the cosmic web is proposed. The large scale environment is classified into four web types: voids, sheets, filaments and knots. The classification is based on the evaluation of the deformation tensor, i.e. the…

Astrophysics · Physics 2010-11-02 J. E. Forero-Romero , Y. Hoffman , S. Gottloeber , A. Klypin , G. Yepes

A fundamental hypothesis for the interpretation of the measured large-scale line-of-sight peculiar velocities of galaxies is that the large-scale cosmic flows are irrotational. In order to assess the validity of this assumption, we…

Astrophysics · Physics 2009-09-25 C. Pichon , F. Bernardeau

The Lagrangian dynamics of a single fluid element within a self-gravitational matter field is intrinsically non-local due to the presence of the tidal force. This complicates the theoretical investigation of the non-linear evolution of…

Cosmology and Nongalactic Astrophysics · Physics 2016-03-23 Xin Wang , Alex Szalay
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