10.1007/978-3-642-25249-5_3
Van De Weygaert, Rien
Rien
Van De Weygaert
Vegter, Gert
Gert
Vegter
Edelsbrunner, Herbert
Herbert
Edelsbrunner0000-0002-9823-6833
Jones, Bernard
Bernard
Jones
Pranav, Pratyush
Pratyush
Pranav
Park, Changbom
Changbom
Park
Hellwing, Wojciech
Wojciech
Hellwing
Eldering, Bob
Bob
Eldering
Kruithof, Nico
Nico
Kruithof
Bos, Patrick
Patrick
Bos
Hidding, Johan
Johan
Hidding
Feldbrugge, Job
Job
Feldbrugge
Ten Have, Eline
Eline
Ten Have
Van Engelen, Matti
Matti
Van Engelen
Caroli, Manuel
Manuel
Caroli
Teillaud, Monique
Monique
Teillaud
Gavrilova, Marina
Marina
Gavrilova
Tan, Kenneth
Kenneth
Tan
Mostafavi, Mir
Mir
Mostafavi
Alpha, Betti and the Megaparsec Universe: On the topology of the Cosmic Web
LNCS
Springer
2011
2018-12-11T12:02:44Z
2019-08-02T12:38:09Z
book_chapter
https://research-explorer.app.ist.ac.at/record/3335
https://research-explorer.app.ist.ac.at/record/3335.json
1306.3640
We study the topology of the Megaparsec Cosmic Web in terms of the scale-dependent Betti numbers, which formalize the topological information content of the cosmic mass distribution. While the Betti numbers do not fully quantify topology, they extend the information beyond conventional cosmological studies of topology in terms of genus and Euler characteristic. The richer information content of Betti numbers goes along the availability of fast algorithms to compute them. For continuous density fields, we determine the scale-dependence of Betti numbers by invoking the cosmologically familiar filtration of sublevel or superlevel sets defined by density thresholds. For the discrete galaxy distribution, however, the analysis is based on the alpha shapes of the particles. These simplicial complexes constitute an ordered sequence of nested subsets of the Delaunay tessellation, a filtration defined by the scale parameter, α. As they are homotopy equivalent to the sublevel sets of the distance field, they are an excellent tool for assessing the topological structure of a discrete point distribution. In order to develop an intuitive understanding for the behavior of Betti numbers as a function of α, and their relation to the morphological patterns in the Cosmic Web, we first study them within the context of simple heuristic Voronoi clustering models. These can be tuned to consist of specific morphological elements of the Cosmic Web, i.e. clusters, filaments, or sheets. To elucidate the relative prominence of the various Betti numbers in different stages of morphological evolution, we introduce the concept of alpha tracks. Subsequently, we address the topology of structures emerging in the standard LCDM scenario and in cosmological scenarios with alternative dark energy content. The evolution of the Betti numbers is shown to reflect the hierarchical evolution of the Cosmic Web. We also demonstrate that the scale-dependence of the Betti numbers yields a promising measure of cosmological parameters, with a potential to help in determining the nature of dark energy and to probe primordial non-Gaussianities. We also discuss the expected Betti numbers as a function of the density threshold for superlevel sets of a Gaussian random field. Finally, we introduce the concept of persistent homology. It measures scale levels of the mass distribution and allows us to separate small from large scale features. Within the context of the hierarchical cosmic structure formation, persistence provides a natural formalism for a multiscale topology study of the Cosmic Web.