The CMB Dipole and Circular Galaxy Distribution
| dc.creator | Tomozawa, Yukio | |
| dc.date | 2007-01-05 | |
| dc.date | 2007-05-16 | |
| dc.date.accessioned | 2026-07-07T10:36:46Z | |
| dc.date.available | 2026-07-07T10:36:46Z | |
| dc.description | The validity of Hubble's law defies the determination of the center of the big bang expansion, even if it exists. Every point in the expanding universe looks like the center from which the rest of the universe flies away. In this article, the author shows that the distribution of apparently circular galaxies is not uniform in the sky and that there exists a special direction in the universe in our neighborhood. The data is consistent with the assumption that the tidal force due to the mass distribution around the universe center causes the deformation of galactic shapes depending on its orientation and location relative to the center and our galaxy. Moreover, the cmb dipole data can also be associated with the center of the universe expansion, if the cmb dipole at the center of our supercluster is assumed to be due to Hubble flow. The location of the center is estimated from the cmb dipole data. The direction to the center from both sets of data is consistent and the distance to the center is computed from the cmb dipole data. | |
| dc.description | 9 pages, 3 figures (10 figure captions), 1 table | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0701151 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0701151 | |
| dc.identifier | Mod.Phys.Lett.A22:1553-1568,2007 | |
| dc.identifier | doi:10.1142/S0217732307023936 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/180165 | |
| dc.subject | Astrophysics | |
| dc.title | The CMB Dipole and Circular Galaxy Distribution | |
| dc.type | text |