I-The Expanding Universe from the Huge Void Center: Theory & Modelling
| dc.creator | Lorenzi, Luciano | |
| dc.date | 1999-06-17 | |
| dc.date.accessioned | 2026-07-25T21:10:29Z | |
| dc.description | To add to and refine the model presented at the Grado3 meeting, of a radial Hubble expansion from the Bahcall & Soneira huge void center, it is here outlined a formal analytical formulation of the theory and modelling on which the previous check work based itself. The new Hubble Law contains the distance R from the expansion center, multiplied by an angular function, and the H's variation, whose meaning and expression have been obtained and examined through a Galaxy Hubble law analysis based on derivatives with respect to light-space. This H's variation, as predicted by the model, is due to a combination of two dominant effects, respectively time (TE) and space (SE). Structurally the scattering noise of the nearby Universe Hubble ratios seems to be partially caused by a perturbative term. In conclusion a fundamental confirmation test of the model is presented. As a physical result, one obtains a higher matter density of the Universe. | |
| dc.description | 24 pages in TeX, 1 figure, presented at the "XLIII Congresso Nazionale Della Societa' Astronomica Italiana - Le Rivoluzioni in Astronomia - Napoli, 4-8 maggio 1999 Osservatorio Astronomico di Capodimonte" | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9906290 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9906290 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/76929 | |
| dc.subject | Astrophysics | |
| dc.title | I-The Expanding Universe from the Huge Void Center: Theory & Modelling | |
| dc.type | text |