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Statistics of cosmological fields

Published online by Cambridge University Press:  01 July 2015

Sabino Matarrese
Sabino Matarrese*
Affiliation:
Dipartimento di Fisica e Astronomia “G. Galilei”, Università degli Studi di Padova and INFN Sezione di Padova, via Marzolo 8, 35131 Padova, Italy Gran Sasso Science Institute, INFN, viale F. Crispi 7, 67100 L'Aquila, Italy email: sabino.matarrese@pd.infn.it
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Abstract

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The general problem of the statistics of the primordial curvature perturbation field in cosmology is reviewed. The search for non-Gaussian signatures in cosmological perturbations, originated from inflation in the early Universe is discussed both from the theoretical point of view and in connection with constraints coming from recent observations and future prospects for observing/constraining them.

Keywords

Cosmology: early Universe: InflationCosmic Microwave Background RadiationLarge Scale Structure of Universenon-Gaussianity
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Symposium S306: Statistical Challenges in 21st Century Cosmology , May 2014 , pp. 116 - 123
Copyright
Copyright © International Astronomical Union 2015 

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