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Primordial non-Gaussianity



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Recording Details

Speaker(s): 
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PIRSA Number: 
07090001

Abstract

The non-Gaussianity of the primordial cosmological perturbations will be strongly constrained by future observations like Planck. It will provide us with important information about the early universe and will be used to discriminate among models. I will review how different models of the early universe can generate different amount and shapes of non-Gaussianity.