File:Cosmic Topology fig4b.jpg
From Scholarpedia

Size of this preview: 703 × 600 pixels.
Original file (980 × 836 pixels, file size: 87 KB, MIME type: image/jpeg)
The Cosmic Crystallography Method in the Poincaré Dodecahedral Space. In this histogram for pairwise separations calculated in a PDS with $\Omega_0 = 1.1$, the presence of spikes signals a multi-connected topology, their positions reflect the size of the fundamental domain (a dodecahedron), and their relative heights characterizes the group of transformations that glue together the opposite faces of the dodecahedron. Although the main spike is situated at a spectral shift too large to be detectable, the first one is at $z \approx 1.5$, accessible to the deep observational surveys expected in this decade.
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 10:09, 18 December 2014 | ![]() | 980 × 836 (87 KB) | Olivier Minazzoli (Talk | contribs) | The Cosmic Crystallography Method in the Poincaré Dodecahedral Space. In this histogram for pairwise separations calculated in a PDS with $\Omega_0 = 1.1$, the presence of spikes signals a multi-connected topology, their positions reflect the size of ... |
- Edit this file using an external application (See the setup instructions for more information)
File usage
The following page links to this file: