|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 listsPMRFPS's The Faraday Institute for Science and Religion The Oon Lectures
Other talksHONORARY FELLOWS LECTURE - Molecules against cancer or for very long term memory Being Different: what difference does diversity make? Structure-based design of vaccines for HIV-1 and RSV Café Synthetique Three Standing Figures - from stone, to studio, to the open air Rail Exclusive - DfT