|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 listsSymposium on Computational Biology Graduate Students at CUED (GSCUED) Events Faculty of Music Colloquia
Other talksThe prospects for thin film PV solar energy in a world dominated by crystalline silicon "Designing trials to find the right dose" Koopman operator theory in fluid mechanics Variation in measures and markers of timeliness of diagnosis in cancer Tuberculous Granuloma Formation and Function Queues don’t matter when you can Jump them!