This book demonstrates for the first time, using state-of-the-art computer simulations, that the interpretation of future galaxy survey measurements is far more subtle than assumed, and that a major revision to our models of these effects is urgently needed.

Essential contribution to the future analysis of galaxy survey data

Has already impacted on the design of major forthcoming missions

Nominated as an outstanding contribution by the University of Durham

Essential contribution to the future analysis of galaxy survey data Has already impacted on the design of major forthcoming missions Nominated as an outstanding contribution by the University of Durham Includes supplementary material: sn.pub/extras

Zusammenfassung
Essential contribution to the future analysis of galaxy survey data

Has already impacted on the design of major forthcoming missions

Nominated as an outstanding contribution by the University of Durham

Inhalt
Introduction.- The Growth of Matter Perturbations in the Universe.- Simulations of Quintessential Cold Dark Matter.- Modelling Redshift Space Distortions in Hierarchical Cosmologies.- Testing Gravity Using the Growth of Large Scale Structure in the Universe.- Conclusions.- Appendices.