Fractal local galaxy number counts may imply strong bias
| dc.creator | Matravers, David | |
| dc.date | 1998-08-05 | |
| dc.date | 1998-09-25 | |
| dc.date.accessioned | 2026-07-07T03:32:35Z | |
| dc.date.available | 2026-07-07T03:32:35Z | |
| dc.description | Exact Tolman solutions are used to analyse the implications if the galactic number has a fractal form out to a distance of about 150 Mpc in a universe which is homogeneous on the large scale. It is concluded that such a model requires either a non-linear Hubble law or a very low density if galaxies trace the total matter distribution. | |
| dc.description | Minor correction to abstract and two references corrected. To appear in the Proceedings of the International Seminar on Mathematical Cosmology, Potsdam, 30 March-4 April 1998, ed. M. Rainer and H-J Schmidt, World Scientific PC. 7 pages LaTeX, sproc style, no figures | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9808015 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9808015 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/36287 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Fractal local galaxy number counts may imply strong bias | |
| dc.type | text |