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A Numerical Renormalization Solution for...
Preprint

A Numerical Renormalization Solution for Self-Similar Cosmic Structure Formation

Abstract

We present results of a numerical renormalization approximation to the self- similar growth of clustering of pressureless dust out of a power-law spectrum

Authors

Couchman HMP; Peebles PJE

Publication date

August 25, 1997

DOI

10.48550/arxiv.astro-ph/9708230

Preprint server

arXiv