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The CMB bispectrum from recombination

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If you have a question about this talk, please contact Camille Bonvin.

CMB non-Gaussianity can be used to discriminate between models of the early universe. However, the primordial signal will be biased by intrinsic non-linearties. I will compute the CMB 3 -p function generated by second-order effects at recombination and discuss their observability and contamination to measurement of primordial signal.

This talk is part of the Cosmology Lunch series.

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