activity
19931997
most citedScaling in the Universe

84 citations · 148 across the 7 of their papers we have counts for

collaborators

7 papers

hep-ph1997★ 2 cited

Dark Matter and the Scale of SUSY Breaking

Stefano Borgani, Antonio Masiero

We review the prospects for dark matter (DM) in two classes of supersymmetric (SUSY) models which are characterized by the different mechanism of SUSY breaking, namely the more com…

astro-ph1995★ 16 cited

The Cluster Distribution as a Test for Dark Matter Models. II: The Dipole Structure

P. Tini Brunozzi, S. Borgani, M. Plionis +2

We study the dipole for a redshift sample of Abell/ACO clusters. To elucidate the constraints it places on dark matter models, we use numerical simulations based on the Zel'dovich…

astro-ph1995★ 18 cited

The Cluster Distribution as a Test for Dark Matter Models. I: Clustering Properties

S. Borgani, M. Plionis, P. Coles +1

We present simulations of the cluster distribution in several dark matter models, using an optimized version of the truncated Zel'dovich approximation (TZA). We compare them with N…

astro-ph1995★ 4 cited

MASS SEGREGATION IN DARK MATTER MODELS.

A. Campos, G. Yepes, A. Klypin +3

We use the moments of counts of neighbors as given by the Generalized Correlation Integrals, to study the clustering properties of Dark Matter Halos (DH) in Cold Dark Matter (CDM)…

astro-ph1994★ 84 cited

Scaling in the Universe

Stefano Borgani

The aim of this review article is to give a comprehensive description of the scaling properties detected for the distribution of cosmic structures. Due to the great variety of stat…

astro-ph1993★ 12 cited

Cluster Correlations in the Zel'dovich Approximation

S. Borgani, P. Coles, L. Moscardini

We show how to simulate the clustering of rich clusters of galaxies using a technique based on the Zel'dovich approximation. This method well reproduces the spatial distribution of…

astro-ph1993★ 12 cited

Non-Linear Clustering in the Cold+Hot Dark Matter Model

S. A. Bonometto, S. Borgani, S. Ghigna +2

We use high resolution PM N-body simulations to follow the development of non-linear clustering in a flat Universe, dominated by Cold + Hot Dark Matter (CHDM) with 60% of CDM, 30%…