Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.285..459r&link_type=abstract
Astrophysics and Space Science, v. 285, Issue 2, p. 459-470 (2003).
Astronomy and Astrophysics
Astrophysics
Scientific paper
The work described in this paper has its origins in a speculation on the realization of Mach's Principle specifically, in the formulation of two questions: (a) Can a globally inertial space & time be associated with a non-trivial global matter distribution? (b) If so, what are the general properties of such a global distribution?This analysis (Roscoe, [2002a] (astro-ph/0107397)), led us to conclude that a globally inertial space & time can be associated with a non-trivial global matter distribution, and that this distribution is necessarily fractal with D=2; that is mass ˜ R 2. Gravitational processes are then to be understood in terms of perturbations of this equilibrium space-matter-time structure. We give a very brief overview of these gravitational processes, specifically applied to spiral galaxies. These considerations led directly to the discovery of a completely new phenomenology in spiral discs reported in detail in Roscoe [2002b] (astro-ph/0107300). We review this phenomenology, and give a brief account of its theoretical explanation.
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