title: Cosmic lacunarity.
abstract: The present distribution of galaxies in space is a remnant of their formation and interaction. On a large enough scale, we may represent the galaxies as a set of points and quantify the structures in this set by its generalized dimensions [Beck and Schlogl, Thermodynamics of Chaotic Systems (Cambridge University Press, Cambridge, 1986); Paladin and Vulpiani, Phys. Rep. 156, 147 (1987)]. The results of such evaluation are often taken to be evidence of a fractal (or multifractal) distribution of galaxies. However, those results, for some scales, may also reveal the presence of singularities formed in the gravitational processes that produce structure in the galaxy distribution. To try to make some decision about this issue, we look for the more subtle galactic lacunarity. We believe that this quantity is discernible in the currently available data and that it provides important evidence on the galaxy formation process. (c) 1997 American Institute of Physics.
authors.affiliation: Istituto di Cosmogeofisica, Corso Fiume 4, I-10133 Turin, Italy.
authors.forename: A.
authors.initials: A
authors.lastname: Provenzale
authors.forename: E. A.
authors.initials: EA
authors.lastname: Spiegel
authors.forename: R.
authors.initials: R
authors.lastname: Thieberger