1993/11/30 by P. M. Harrington, Harrington, P. M., Adrian L. Melott +4
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #Adhesion, Friction, and Surface Interactions #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph #nanoparticles nucleation surface interactions
paper · pdf · doi:10.48550/arxiv.astro-ph/9311076
5 pages of Tex plus 5 Postscript figures in compressed uuencoded tar file
openalex publication_date 1993/11/30 · arxiv created 1993/12/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We present in this paper a quantitative method for defining void size in large-scale structure based on percolation threshold density. Beginning with two-dimensional gravitational clustering simulations smoothed to the threshold of nonlinearity, we perform percolation analysis to determine the large scale structure. The resulting objective definition of voids has a natural scaling property, is topologically interesting, and can be applied immediately to redshift surveys.