|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 listsAAAS members and friends event Thinking Society: What is Life? Chinese Culture Events
Other talksEmission line mapping of galaxies at high resolution: optical radioastronomy The Evolution of Arthropods: From Limb Transformation in Crustaceans to Color Variation in Butterflies Presentation: Challenge 4. Making Decisions Using Uncertain Forecasts Arborescent knots, mutants - current status on their invariants A feast of languages: multilingualism in neuro-typical and atypical populations Group Discussions (Isaac Newton Institute & Centre for Mathematical Sciences)