Primordial Non-Gaussianities from Inflation Models
arXiv:1002.1416 · doi:10.1155/2010/638979
Abstract
This is a pedagogical review on primordial non-Gaussianities from inflation models. We introduce formalisms and techniques that are used to compute such quantities. We review different mechanisms which can generate observable large non-Gaussianities during inflation, and distinctive signatures they leave on the non-Gaussian profiles. They are potentially powerful probes to the dynamics of inflation. We also provide a non-technical and qualitative summary of the main results and underlying physics.
84 pages, invited review for special issue of Advances in Astronomy on "Testing the Gaussianity and Statistical Isotropy of the Universe"; v3, various improvement and corrections, especially in Sec.6.4, 8.1 & 9.2
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