Regularity of the large-scale structure of the Universe
| dc.creator | Einasto, J. | |
| dc.date | 1997-11-26 | |
| dc.date.accessioned | 2026-07-07T02:25:25Z | |
| dc.date.available | 2026-07-07T02:25:25Z | |
| dc.description | The distribution of Abell-ACO clusters of galaxies shows that clusters located in rich superclusters form a quasiregular network with step size 120 Mpc. The power spectrum of clusters of galaxies has a sharp peak at a wavelength equal to the step size of the network, the correlation function of clusters is oscillating with this period. We show that spectra with a spike are in agreement with temperature anisotropies measured by the Saskatoon experiment. The corresponding initial power spectrum of matter has a peak followed by a break. | |
| dc.description | 9 pages, 4 ps figures, LaTeX, uses crckapb.sty; Cosmological Parameters and Evolution of the Universe (IAU Symposium 183) ed. K Sato, Kluwer Academic Publ. (in press) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9711321 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9711321 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11864 | |
| dc.subject | Astrophysics | |
| dc.title | Regularity of the large-scale structure of the Universe | |
| dc.type | text |