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The CMB bispectrum from recombination
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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Other listsCambridge Parasitology Club Meetings 2012-13 GBR talks Martin Centre Research Seminars, Dept of Architecture
Other talks‘Pfizer Chemical and Biological Synthesis and Catalysis Symposium 2015’ (students from both the Biological and Synthetic RIGS will be interested in this Symposium) Making Shale Oil and Gas Production Safer and More Efficient Technology Development Structure of the mitochondrial ATPase Doing social research with social media: the question of participation Lava, luck and linear logs