|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 listsReading Group on Stochastic Differential Equations Cambridge Biomedical Research Centre "Distinguished Visitors" 2015 Lecture Series Kettle's Yard ARTcrowd
Other talksS7 - Probing the physics of AGN through integral field spectroscopy A novel gene essential for the generation of reactive oxygen species and host defence Investigation of priming effects on associative memory TBA Pitch perception: New approaches to classic questions Hierarchical Structuring of Carbon Nanotubes