Abstract
We discuss how primordial non-Gaussianity of the curvature perturbation helps to constrain models of the early universe. Observations are consistent with Gaussian initial conditions, compatible with the predictions of the simplest models of inflation. Deviations are constrained to be at the sub percent level, constraining alternative models such as those with multiple fields, non-canonical kinetic terms or breaking the slow-roll conditions. We introduce some of the most important models of inflation which generate non-Gaussian perturbations and provide practical tools on how to calculate the three-point correlation function for a popular class of non-Gaussian models. The current state of the field is summarised and an outlook is given.
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Acknowledgements
Christian T. Byrnes is supported by a Royal Society University Research Fellowship. I wish to thank the organisers of the second JPBCosmo school for the invitation to hold this lecture course in the shadow of the beautiful Pedra Azul mountain in EspÃrito Santo, Brasil. Special thanks are due to Hermano Endlich Schneider Velten and his family for hospitality before and after the school.
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Byrnes, C.T. (2016). Lecture Notes on Non-Gaussianity. In: Fabris, J., Piattella, O., Rodrigues, D., Velten, H., Zimdahl, W. (eds) The Cosmic Microwave Background. Astrophysics and Space Science Proceedings, vol 45. Springer, Cham. https://doi.org/10.1007/978-3-319-44769-8_3
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