|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 listsCUEX Presents: On Foot Across China And Other Human Powered Adventures Culture of Scientific Research Institute of Biotechnology Seminar Series
Other talksDecoding human genomes on a population scale DEPARTMENTAL RESEARCH DAY tba A Glance at the Exotic Quantum Liquids and Solids of the Two-Dimensional Electron Gas Manipulation of biochemical pathways in plants Tatous and Taiwan Devils: making sense of scaly mammals in the seventeenth century