|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
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.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other listsInformal Theoretical Geophysics Lunchtime Seminars (DAMTP) Statistical Laboratory International Year of Statistics Public Lectures Qatar Carbonates and Carbon Storage Research Centre: Status update after three years of fundamental research
Other talksMechanisms regulating tumor heterogeneity Is the Future of Electronics Packaging in 3D Printing CNE meeting On the Indian origins of Nationalism Soft Matter Challenges - Oil and Gas Sector Inhibition of phagocytosis by extracellular pathogens enteropathogenic and enterohaemorrhagic Escherichia coli