I-The Expanding Universe from the Huge Void Center: Theory & Modelling
Abstract
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.
Cite
@article{arxiv.astro-ph/9906290,
title = {I-The Expanding Universe from the Huge Void Center: Theory & Modelling},
author = {Luciano Lorenzi},
journal= {arXiv preprint arXiv:astro-ph/9906290},
year = {2007}
}
Comments
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"