A Three Dimensional Percolation Analysis of the Topology of the Las Campanas Redshift Survey.

Details A Three Dimensional Percolation Analysis of the Topology of the Las Campanas Redshift Survey. A Three Dimensional Percolation Analysis of the Topology of the Las Campanas Redshift Survey.

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aps..apr..i703y&link_type=abstract

American Physical Society, APS/AAPT Joint April Meeting, April 18-21, 1998 Columbus, Ohio, abstract #I7.03

Physics

Scientific paper

We present in this talk a 3-D percolation analysis of the topology of the Las Campanas Redshift Survey. Percolation analysis has been developed, over the last decade, as a sensitive tool for describing the topology of galaxy distributions. The analysis can distinquish between clumpy and connected distributions of galaxies for surveys which have very different geometries or selection criteria. The topology of galaxy distributions has implications for theories of large scale structure developement.

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