Cosmological Bootstrap, with and without Spin
I will describe the Cosmological Bootstrap – an approach to compute correlation functions of primordial fluctuations based on symmetries and singularities. Using this approach, I will present some new results for inflationary three and four-point functions of scalars and tensors. These shapes do not depend on the specific inflationary model, as long as the fluctuations minimally break de Sitter symmetry.
University of Amsterdam
Speaker
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Gui Pimentel
