Cosmic Expansion vs. Galactic Density

From Natural Philosophy Wiki
Revision as of 11:18, 30 December 2016 by Maintenance script (talk | contribs) (Imported from text file)
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
Jump to navigation Jump to search
Scientific Paper
Title Cosmic Expansion vs. Galactic Density
Read in full Link to paper
Author(s) Raymond H Gallucci
Keywords Galactic Density; Cosmic Expansion; Simulation; Steady-State
Published 2015
No. of pages 4

Read the full paper here

Abstract

Observing galactic density as a function of increasing distance (and, correspondingly, earlier times given the travel time of light) should provide evidence as to whether a ‘steady-state’ (non-expanding) or Big-Bang-driven expanding universe is the more defensible cosmology. Working independently, but later discovering additional recent work in this area by Heymann, I attempt to address this question by simulating galactic densities for the two types of cosmological model. Results suggest that the non-expanding universe may be more consistent, or at least less inconsistent, with both observation and expectation. Further, they are consistent with conclusions drawn by Heymann from his recent studies.