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Hot gas in galaxy clusters: Theory and simulations
M. L. Norman
1 - 35
10.3254/978-1-61499-015-4-1
Proceedings of the International School of Physics "Enrico Fermi"
Volume 159: Background Microwave Radiation and Intracluster Cosmology
Abstract

1. Introduction

2. Cosmological framework and perturbation growth in the linear regime

3. Analytic models for non-linear growth, virial scaling relations, and halo statistics

4. Numerical simulations of gas in galaxy clusters

5. Comparisons and predictions for X-ray and SZE surveys

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